@jartsa My wording will be a bit different from that of the experts around here, being not one of those.
Let's compare two boxes, box A, the not expanding box, is glued so that the proper distance between the mirrors is constant over time. Box B, the expanding box is not glued, so that the proper distance between the mirrors increases according to to the expansion of the universe (more precisely proportional to the increasing scale factor).
Now imagine the two boxes side by side. After the light pulses has been emitted at one side (let's call this side of the box "pulse emitting side") we measure the frequency shift at the opposite mirrors.
The opposite mirror in box B moves away from the "pulse emitting side" while the light is traveling and we measure a redshift at this mirror corresponding to the expansion of the universe. This mirror "moves away" because it is comoving (from it's view the universe is homogeneous and isotropic).
The opposite mirror in box A can't move away from the "pulse emitting side" , so this mirror moves relative to the opposite mirror of box B towards the "pulse emitting side". Now imagine a comoving observer just before passing by. From the opposite mirror's (still box A) view this observer is blueshifted by the same amount of frequency shift as this observer sees the emitting side redshifted. Putting this together the emitting side of the box A is seen with zero frequency shift from the view of the opposite side of the box A as it should be because this box is not expanding.
Note, this presupposes that homogeneity and isotropy of the universe holds at all scales.
For simplicity it is assumed that the "emitting side" of both boxes is comoving.
It's my trial, dear experts please correct where necessary.