The galaxy presents as a somewhat elliptical, though not perfectly spherical, system. There is a high degree of central concentration with a bright, unresolved core. The light profile appears relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. A faint, diffuse halo surrounds the central region, gradually fading into the background. There are hints of slight disturbances or tidal features in the outer regions, but they are not highly pronounced, indicating potential minor gravitational interactions with neighboring galaxies or past merger events. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy undergoing a low rate of star formation. The color indices suggest a population dominated by older stars, though some blue light indicates that there is some star formation taking place.
