The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge that is bright and appears yellow to white in color, possibly indicating an older stellar population. The outer regions show a gradual decrease in surface brightness and a bluish hue, suggesting the presence of some younger, bluer stars or possibly ongoing, albeit limited, star formation. The overall shape deviates somewhat from being perfectly round, leaning towards an elongated, cigar-like appearance, but is predominantly elliptical. There are no obvious signs of tidal tails, disrupted morphology, or ongoing major mergers. The galaxy appears relatively isolated and undisturbed.
