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Observations of the pair of galaxies VV 330 with the SCORPIO multimodeinstrument on the 6-m Special Astrophysical Observatory telescope arepresented. Large-scale velocity fields of the ionized gas in H-alfa andbrightness distributions in continuum and H-alfa have been constructed for bothgalaxies with the help of a scanning Fabry Perot interferometer. Long-slitspectroscopy is used to study the stellar kinematics. Analysis of the dataobtained has revealed a complex structure in each of the pair components. Threekinematic subsystems have been identified in UGC 5600: a stellar disk, an innergas ring turned with respect to the disk through ~80degrees, and an outer gasdisk. The stellar and outer gas disks are noncoplanar. Possible scenarios forthe formation of the observed multicomponent kinematic galactic structure areconsidered, including the case where the large-scale velocity field of the gasis represented by the kinematic model of a disk with a warp. The velocity fieldin the second galaxy of the pair, UGC 5609, is more regular. A joint analysisof the data on the photometric structure and the velocity field has shown thatthis is probably a late-type spiral galaxy whose shape is distorted by thegravitational interaction, possibly, with UGC 5600.

2D Spectroscopy of Candidate Polar-Ring Galaxies: I. The Pair of Galaxies UGC 5600/09