The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. It exhibits a generally elongated shape, appearing somewhat cigar-shaped. There is a color gradient from the core outwards, with the central region displaying a yellowish-white hue, suggesting an older stellar population. The outer regions transition to a bluer color, possibly indicating younger stars or ongoing star formation, though at a low rate. There is no obvious evidence of significant spiral arm structure or major disturbances due to mergers, although there may be minor asymmetric features.
