  We measured the velocity curve and the velocity dispersion profile of the
ionized gas along the major axis of the edge-on galaxy UGC~10205. The observed
kinematics extends up to about 40 arcsec from the nucleus. In the inner 13
arcsec of this early-type spiral three kinematically distinct gaseous
components are present. We disentangle a fast-rotating and a slow-rotating
component. They give to the UGC10205 velocity curve a ``figure-of-eight''
appearance.
  A third velocity component is also detected on the southeast side of the
galaxy. Possibly it is produced by gas in non-circular motions.
