  We introduce a two-parameter static, nonspherically-symmetric black hole
solution in the Einstein theory of gravity coupled with a massless scalar
field. The scalar field depends only on the polar coordinate $\theta$ in the
spherical coordinates representation. The scalar invariant of the spacetime,
namely, the Kretschmann scalar reveals that the black hole is singular on its
axis of symmetry for all nonzero values of the scalar charge. It also manifests
two surfaces of singularity for a certain interval of the value of the scalar
charge. These singularities are hidden behind the event horizon's surface
except the singularity on the axis which is naked. The energy-momentum of the
scalar field satisfies all energy conditions. A simple investigation reveals
that the circular orbit of massive and massless particles in the equatorial
plane is identical to the Schwarzschild black hole.
