  The exact axisymmetric and static solution of the Einstein equations coupled
to axisymmetric and static gravitating scalar (or phantom) field is presented.
The spacetimes modified by the scalar field are explicitly given for the so
called $\gamma$-metric and Erez-Rosen metric with quadrupole moment $q$,
influence of the additional deformation parameters $\gamma_*$ and $q_*$
generated by the scalar field is studied. It is shown that the null energy
condition is satisfied for the phantom field, but it is not satisfied for the
standard scalar field. The test particle motion in the both modified
$\gamma$-metric and Erez-Rosen quadrupole metric is studied; the circular
geodesics are determined, and near-circular trajectories are explicitly
presented for characteristic values of the spacetime parameters. It is also
demonstrated that the parameters $\gamma_*$ and $q_*$ have no influence on the
test particle motion in the equatorial plane.
