The galaxy presents as a somewhat diffuse, yellowish object with a generally elliptical morphology. The light distribution appears relatively smooth, although there are some subtle signs of substructure that could indicate ongoing or past interactions. Specifically, there is a slight extension or asymmetry noticeable at the apparent base, possibly indicative of a tidal tail or remnant of a minor merger. The galaxy's core appears brighter and more concentrated than its outer regions, with a suggestion of a central bulge. Overall the galaxy seems to be a relatively evolved system. There are hints of dusty patches or regions of enhanced star formation, but these are not prominent, suggesting a low star formation rate.
