The galaxy appears as a single, somewhat centrally concentrated object. The morphology is smooth, with a general lack of distinct spiral arms or other features typically associated with late-type galaxies. The galaxy's light distribution suggests a centrally concentrated bulge surrounded by a fainter, more diffuse halo or disk. Color gradients appear to be present, with a yellower core and bluer outskirts. There are no signs of strong tidal features or ongoing mergers, although some subtle asymmetries or minor disturbances cannot be ruled out. The galaxy has an elliptical shape, with its major axis slightly longer than its minor axis. It exhibits a centrally concentrated profile, suggesting a significant bulge component.
