The galaxy presents as a generally smooth, elliptical morphology, with a high degree of central concentration. It exhibits a predominantly yellowish hue, suggestive of an older stellar population and diminished recent star formation. The galaxy appears nearly circular, showing little to no disk-like structure or significant tidal features. There are subtle hints of substructure within the galaxy, with a slightly elongated, irregular shape and some brighter regions that suggest a recent minor disturbance. There are two distinct orange regions, and the galaxy is generally more concentrated than other observed objects in the vicinity.
