The galaxy presents a generally smooth and centrally concentrated appearance. There is a suggestion of a slightly elongated form, though it leans towards being relatively round. Its color is predominantly reddish-yellow, indicative of an older stellar population and a lower rate of active star formation. There are no obvious signs of a spiral structure or prominent dust lanes. Close inspection suggests a very slight asymmetry in its shape, perhaps indicative of a minor gravitational interaction or past merger event, but overall, it appears to be largely undisturbed. The galaxy is moderately luminous, likely a galaxy with a substantial mass, and the redder hue suggests it is relatively mature in its evolutionary stage.
