This galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a predominantly elliptical morphology. There is a lack of discernible spiral arm structure or prominent dust lanes. The galaxy displays a yellowish-orange hue, suggestive of an older stellar population. The light profile appears to gradually decrease from the central region outwards, with no sharp edges or distinct features. The overall shape deviates slightly from perfectly round, appearing more ellipsoidal. There is a possible minor disturbance or interaction in the lower part of the galaxy, with a slightly bluer region in the outer disk. The general structure indicates that the galaxy is likely an evolved system with a relatively low star formation rate.
