I've found an answer in a comment on Lo (2002) by Mertens (2002) that I can understand and have listed some additional steps below. The approach is slightly different to what I've listed in the original question but the results are exactly the same. The argument goes as follows: dropping Lo's assumption of normality introduces skewness and excess kurtosis in the asymptotic variance of the moment estimator. To get to this result, we use GMM.
Let $\theta= \left[\mu \ \ \sigma^2 \right]'=\begin{bmatrix}\mathbb E[R_t] \\ \mathbb E[(R_t-\mu)^2] \end{bmatrix}$ and aim to solve the following (using GMM):
$$
H(\theta) = \begin{bmatrix}
R_t-\mu \\
(R_t-\mu)^2-\sigma^2 \\
\end{bmatrix}
$$
$$f(H(\theta)) = \frac{1}{T}\sum^T_{t=1} H_t(\theta)\stackrel{!}{=}0$$
This is solved over the entire data set $T$ but I've dropped some notation for ease from the original paper. The variance-covariance matrix of $H$ is then:
$$
S=\mathbb E\left[H(\theta)H(\theta)'\right]= \mathbb E
\begin{bmatrix}
(R_t-\mu)^2 && (R_t-\mu)\left((R_t-\mu)^2-\sigma^2\right) \\
(R_t-\mu)\left((R_t-\mu)^2-\sigma^2 \right) && \left((R_t-\mu)^2-\sigma^2) \right)^2\\
\end{bmatrix}
$$
Multiplying out and evaluating the expectations we get:
$$
S=
\begin{bmatrix}
\sigma^2 && \mathbb E\left[(R_t-\mu)^3-(R_t-\mu)\sigma^2 \right] \\
\mathbb E\left[(R_t-\mu)^3-(R_t-\mu)\sigma^2 \right] && \mathbb E \left[ (R_t-\mu)^4 - 2\underbrace{(R_t-\mu)^2}_{\sigma^2}\sigma^2 + \sigma^4\right ] \\
\end{bmatrix}
$$
Some terms can be simplified in expectation, notably in the top right and bottom left we have $\mathbb E[(R_t-\mu)\sigma^2]=0$. We then get:
$$
S = \begin{bmatrix} \sigma^2 && \mathbb E\left[(R_t-\mu)^3\right] \\ \mathbb E\left[(R_t-\mu)^3\right] && \mathbb E\left[(R_t-\mu)^4\right] -\sigma^4\end{bmatrix}$$
Next, the delta method applied to the Sharpe Ratio can be written as:
$$V_{SR}=\frac{\partial g}{\partial \theta'}V_\theta \frac{\partial g}{\partial \theta'}'$$
The partial derivatives of the Sharpe Ratio function $g(\theta)=g(\mu,\sigma^2)$ are easy, we get:
$$\frac{\partial g}{\partial \theta'}=\begin{bmatrix} 1/\sigma \\ -\frac{\mu}{2\sigma^3}\\ \end{bmatrix}$$
Finally, we're back to what Opdyke (2005) is doing in his paper and can address the original question. Setting $V_\theta=S$ and multiplying out $V_{SR}$ we get (I've dropped the risk free rate $R_f$):
$$V_{SR}
=\frac{\sigma^2}{\sigma^2}-2\frac{\mu}{2\sigma^3}\frac{1}{\sigma} \mathbb E \left[ (R_t-\mu)^3\right] + \frac{\mu^2}{4\sigma^6} \left( \mathbb E \left[(R_t-\mu)^4\right]-\sigma^4\right)$$
Let $\gamma_3=\frac{\mathbb E \left[(R_t -\mu)^3 \right]}{\sigma^3}$ and $\gamma_4=\frac{\mathbb E \left[(R_t -\mu)^4 \right]}{\sigma^4}$ be the third and fourth standardized, central momements then we get:
$$V_{SR}=1-SR\cdot\gamma_3 + \frac{1}{4}SR^2\cdot (\gamma_4-1)$$
Mertens recovers Lo's result by adding and subtracting $\frac{1}{2}SR^2$ which then, finally, gives us:
$$\boxed{V_{SR}=1+\frac{1}{2}SR^2-SR\cdot\gamma_3 + SR^2\cdot \frac{\gamma_4-3}{4}}$$