  A spherically symmetric solution of the field equations of the
Ho\v{r}ava--Lifshitz gravity--gauge vector interaction theory is obtained and
analyzed. It describes a charged throat. The solution exists provided a
restriction on the relation between the mass and charge is satisfied. The
restriction reduces to the Reissner--Nordstr\"{o}m one in the limit in which
the coupling constants tend to the relativistic values of General Relativity.
We introduce the correct charts to describe the solution across the entire
manifold, including the throat connecting an asymptotic Minkowski space--time
with a singular 3+1 dimensional manifold. The solution external to the throat
on the asymptotically flat side tends to the Reissner--Nordstr\"{o}m
space--time at the limit when the coupling parameter, associated with the term
in the low energy Hamiltonian that manifestly breaks the relativistic symmetry,
tends to zero. Also, when the electric charge is taken to be zero the solution
becomes the spherically symmetric and static solution of the
Ho\v{r}ava--Lifshitz gravity.
