Cosmological measurements suggest that we live in a flat universe. However, what might be less clear is its topology. So could the flat universe have the form of a $T^3$-torus, i.e. the torus whose surface would be (diffeomorph to) 3D ?
For instance the Robertson-Walker metric for $k=0$ could turn out as a $T^3$ if certain point identification would apply.
Or would that contradict the rules of homogeneity and isotropy of the universe which is the basis for the Robertson-Walker metric ? If the latter were not the case, why would it be not possible ?