The galaxy presents a generally smooth and elliptical morphology. Its shape is primarily rounded, tending toward a slightly elongated, cigar-shaped appearance. The light distribution appears concentrated towards the center, with a bright central bulge that is yellowish in color. This indicates a potentially older stellar population in the nucleus. Moving outward from the bulge, the galaxy exhibits a faint disk or halo component.

There appears to be some minor asymmetry or subtle disturbances in the outer regions, which could be indicative of a past or ongoing interaction, although not exhibiting any major merging features. The overall color profile suggests that the galaxy's star formation rate is relatively low, but likely not completely absent. The estimated size and absolute magnitude indicate that it is a relatively large galaxy.
