  In this paper, we present the spherically symmetric Proca star in the
presence of a phantom field and obtain a traversable wormhole solution for
non-trivial topological spacetime. Using numerical methods, symmetric solutions
and asymmetric solutions are obtained in two asymptotically flat regions. We
find that when changing the throat size $r_{0}$, both the mass $M$ and the
Noether charge $Q$ no longer have the spiral characteristics of an independent
Proca star, furthermore, the asymmetric solution can be turned into the
symmetric solution at some frequency $\omega$ in certain $r_{0}$. In
particular, we find that when the frequency takes a certain value, for each
solution, there is an extremely approximate black hole solution, and there is
even a case where an event horizon appears on both sides of the wormhole
throat.
