The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region, characterized by a yellowish-white hue, which suggests a population of older stars. The outer regions of the galaxy display a bluer tint on its left side. The object shows some characteristics that could indicate a spiral structure, such as a possible disk, but it could also just be noise. There is no apparent major interaction or ongoing merger. There also appears to be a small amount of star formation ongoing. The overall shape appears mostly round.
