The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears predominantly yellow/orange. There may be evidence of some disc-like structure, though this is not well defined and appears somewhat distorted. There is a very faint outer halo of diffuse light extending from the central region, but with low surface brightness. There is very little evidence of defined spiral arms or dust lanes. The galaxy seems to be quite isolated with no obvious tidal features indicating ongoing major mergers, though a very small, close companion cannot be ruled out. The overall color suggests an older stellar population and the absence of significant recent star formation.
