Let $\mathbf{R} \ni X_1, \dots, X_n \sim \mathcal{N}(0, \sigma^2)$. I can show that $$ \mathbb{E} ~ \text{Med} \{X_1, \dots, X_n\} = 0 $$ and want to compute the variance of the same sample median, i.e. $$ \mathbb{V}ar ~ \text{Med} \{X_1, \dots, X_n\} $$
I have a guess that it should behave like sample mean ($\asymp \frac {\sigma^2} n$), since everything is symmetric and stuff, but no idea how to show it rigorously.
This is not an answer, but it's too long for a comment.
Clearly, the answer must scale proportionally to $\sigma^2$, so let's just assume $\sigma=1$.
Sampling $x_1, \ldots, x_n$ i.i.d. from a standard Gaussian is equivalent to sampling a random Gaussian vector $\vec{x} \in \mathbb{R}^n$ with mean $\vec{0}$ and identity covariance matrix. The median coordinate $\mathrm{Med}(\vec{x})$ satisfies $$\mathrm{Med}(\vec{x}) = ||\vec{x}|| \mathrm{Med}(\hat{x})$$ where $\hat{x} = \frac{\vec{x}}{||\vec{x}||}$ is the corresponding unit vector.
For Gaussians, the radius and unit vector are independent, so the calculation factors: $$\mathbb{E}_{\vec{x} \sim N(\vec{0}, I)}[\mathrm{Med}(\vec{x})^2] = \mathbb{E}_{r,\ \hat{x} \sim \mathrm{unif}(S^{n-1})}[r^2 \mathrm{Med}(\hat{x})] = \mathbb{E}_r[r^2] \mathbb{E}_{\hat{x} \sim \mathrm{unif}(S^{n-1})}[\mathrm{Med}(\hat{x})^2].$$
Here $r$ is just the norm of $\vec{x}$ so $\mathbb{E}_r[r^2] = \mathbb{E}_{\vec{x}}[||\vec{x}||^2] = n$. The distribution of $\hat{x}$ is uniform on the sphere by symmetry.
I don't know how to calculate this integral over the sphere though. You can do obvious things like dividing by $n!$ and restricting to the sector $U_0 = \{x_1 \leq x_2 \leq \cdots \leq x_n\} \subset S^{n-1}$: $$\mathbb{E}_{\hat{x} \sim \mathrm{unif}(S^{n-1})}[\mathrm{Med}(\hat{x})^2] = n! \int_{\hat{x} \in U_0} (x_{(n+1)/2})^2 d\mu(\hat{x}),$$ but already for $n=5$ Mathematica doesn't manage to compute the integral.