The galaxy presents as a relatively smooth, concentrated object. It exhibits a moderate degree of ellipticity, appearing somewhat elongated but not significantly cigar-shaped. There is evidence of potential interaction or disturbance, possibly a minor tidal feature. The galaxy has a slightly yellowish hue, suggestive of an older stellar population and reduced star formation activity. The overall morphology seems to indicate a galaxy that has largely settled into a stable configuration, with a dominant bulge component.
