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We present our spectroscopic observations of the galaxy NGC 7468 performed atthe 6-m Special Astrophysical Observatory telescope using the UAGS long-slitspectrograph, the multipupil fiber spectrograph MPFS, and the scanningFabry-Perot interferometer (IFP). We found no significant deviations from thecircular rotation of the galactic disk in the velocity field in the regions ofbrightness excess along the major axis of the galaxy (the putative polar ring).Thus, these features are either tidal structures or weakly developed spiralarms. However, we detected a gaseous disk at the center of the galaxy whoserotation plane is almost perpendicular to the plane of the galactic disk. Thecentral collision of NGC 7468 with a gas-rich dwarf galaxy and their subsequentmerging seem to be responsible for the formation of this disk.Comment: 8 pages, 6 figures, accepted in Astronomy Letters, 2004, vol 30., N  9, p. 58

NGC 7468: A galaxy with an inner polar disk