A finite spherical universe of radius R = 13.8 Gly is assumed, with perfect observational reach D = 13.8 Gly in every direction. Each test below places observers at random positions inside that sphere (uniform in volume) and asks whether the universe would look the same - isotropic, self-consistent - from those positions as it does from the centre. It would not, except from a vanishingly small privileged region.
For an observer at distance r from the centre, the ratio of the deepest to the shallowest line of sight to the boundary is A = (R+r)/(R−r). Near-isotropy (A close to 1) requires r to be extremely small relative to R.
Every observer's reach D equals the universe radius R. For an off-centre observer, the observable sphere and the finite universe sphere are not the same sphere. Part of what the observer "sees" lies outside the finite universe; part of the finite universe lies beyond what the observer can see.
A synthetic structured universe is built from cluster nodes, filamentary bridges between them, and a diffuse background - a topology-agnostic stand-in for any structured cosmic web, not a reconstruction of the real sky. The angular, radial, and dipole "sky signature" seen from the centre is compared against the signature seen from many relocated observers.