While reading some questions about the polarisation of a photon, I was wondering about its quantum mechanical representation as a classical vector in the electromagnetic field operator : \begin{equation}\tag{1} \hat{\vec{A}}(t, \vec{r}) = \sum_{k, \, \sigma} \big( \hat{a}_{k,\, \sigma} \, \vec{\varepsilon}_{k, \, \sigma} \, e^{i \vec{k} \cdot \vec{r} \,-\, i \omega_k \, t} + \text{h.c}\big). \end{equation} Here, the polarisation state is represented by a classical vector $\vec{\varepsilon}_{k, \, \sigma}$ in $\mathbb{R}^3$ (or $\mathbb{C}^3$ for the circular polarisation), where $\sigma = \pm 1$ are the two orthogonal circular polarisation states, such that (the wave is transverse): \begin{align}\tag{2} \vec{k} \cdot \vec{\varepsilon}_{k, \, \sigma} &= 0, \\[12pt] \vec{\varepsilon}_{k, \, \sigma}^{\, *} \cdot \vec{\varepsilon}_{k, \, \sigma'} &= \delta_{\sigma \sigma'}. \tag{3} \end{align} The wave's amplitude is an operator : $\hat{a}_{k, \, \sigma}$, with the usual bosonic commutation relations.
Is there a Heisenberg relation on the polarisation states, or is this just a non-sense question since it's a "classical property" of the wave?