The galaxy presents as a relatively smooth, centrally concentrated object. A distinct bulge is visible, exhibiting a yellowish hue. Faint spiral arms emanate from the central bulge, though they are not sharply defined and appear somewhat tightly wound. There is evidence of some bluer regions within the spiral arms, suggesting areas of more recent star formation, though these areas are limited. Overall, the galaxy displays a morphology consistent with a late-type spiral galaxy approaching a lenticular or S0 classification. There is some indication of a potential minor disturbance or tidal feature on one side of the galaxy, suggesting possible interaction with another galaxy.
