  We study a model of spin-1 dark matter which interacts with the Standard
Model predominantly via exchange of Higgs bosons. We propose an alternative UV
completion to the usual Vector Dark Matter Higgs Portal, in which vector-like
fermions charged under SU(2)$_W \times$ U(1)$_Y$ and under the dark gauge
group, U(1)$^\prime$, generate an effective interaction between the Higgs and
the dark matter at one loop. We explore the resulting phenomenology and show
that this dark matter candidate is a viable thermal relic and satisfies Higgs
invisible width constraints as well as direct detection bounds.
