Maxwell's equations describe the electromagnetic field in terms of the vectors
$$
\begin{matrix}
\mathbf{E}(\mathbf{x},t)=(E_x(\mathbf{x},t),E_y(\mathbf{x},t),E_z(\mathbf{x},t)),\\\mathbf{B}(\mathbf{x},t)=(B_x(\mathbf{x},t),B_y(\mathbf{x},t),B_z(\mathbf{x},t))
\end{matrix}$$
whose components are real numbers that also represent the result you would get if you measured the relevant field component at a particular point in spacetime.
In quantum field theory the equations of motion of fields are written in terms of Hermitian operator valued fields called observables. QFT predictions are usually written in terms of correlation functions among the values of the field observables. There are photon number observables whose eigenvalues represent the possible results of measuring the number of photons of a given momentum and polarisation with values corresponding to 0,1,2... photons. This is explained in many quantum field theory books such as "Quantum field theory for the gifted amateur" by Lancaster and Blundell.
Copying information out of a quantum system suppresses interference: this is called decoherence:
https://arxiv.org/abs/1911.06282
There are many papers on the decoherent limit of quantum field theories including QED:
https://arxiv.org/abs/quant-ph/9510021
https://arxiv.org/abs/quant-ph/0210013
For more on the classical limit of quantum field theory see Chapter 8 of "The conceptual framework of quantum field theory" by Anthony Duncan.