The galaxy presents an elliptical morphology, with a smooth light distribution indicating a relatively homogenous stellar population. The central region exhibits a concentrated, bright core suggesting a high stellar density. Proceeding outwards, the galaxy appears more diffuse, with a gradual decrease in luminosity. Faint, irregular structures are subtly detected in the outer regions; however, it is difficult to say what these structures are. Colors are observed with the core appearing more redshifted than the outer components. The galaxy appears to be experiencing moderate star formation, which supports the colors observed. The isophotes are somewhat elongated, deviating slightly from a perfect circle, with the galaxy appearing in-between round and cigar-shaped. No signs of major disturbances or merging events are readily apparent in this image. Overall, the galaxy gives the appearance of an evolved system with ongoing, though not overly intense, stellar formation.
