The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright central region, likely a prominent galactic bulge. The radial color gradient suggests a population of older stars dominating the core, indicated by its yellowish hue. There is a slight deviation from perfect circularity, appearing somewhat elongated in shape, but it does not present any obvious signs of strong tidal interactions or ongoing major mergers, although there are signs of minor disturbances in the galaxy. There is also a faint bluish portion of the galaxy visible on the right side of the image, indicating the possible presence of some younger stars. The galaxy appears relatively isolated, showing no immediate signs of interaction with other nearby galaxies in the field of view. The faintness of any extended disk or halo suggests a relatively quiescent galaxy with a low star formation rate.
