  We present our observations of the galaxy UGS 5600 with a long-slit
spectrograph (UAGS) and a multi-pupil field spectrograph (MPFS) using the 6-m
telescope at Special Astrophysical Observatory. Radial-velocity fields of the
stellar and gaseous components were constructed for the central region and
inner ring of the galaxy. We proved the existence of two almost orthogonal
kinematic subsystems and conclude that UGC 5600 is a galaxy with an inner polar
ring. In the circumnuclear region, we detected noncircular stellar motions and
suspected the existence of a minibar. The emission lines are shown to originate
in H II regions. We estimated the metallicity from the intensity ratio of the
[NII]$\lambda6583$ and \Ha lines to be nearly solar, which rules out the
possibility that the polar ring was produced by the accretion of gas from a
dwarf companion.
