The galaxy presents as a relatively compact object. It exhibits a centrally concentrated luminosity profile, suggesting a significant bulge component. The light appears smooth and diffuse, with no discernible spiral arm structures or prominent dust lanes. The overall shape is generally round, with a slight elongation. There is a subtle color gradient, with the central region appearing slightly yellower compared to the outer regions, which exhibit a bluer hue. No signs of strong tidal disturbances or ongoing major merger events are apparent, although there may be a faint, subtle asymmetry in the outer regions. This galaxy is a system that is likely undergoing low levels of star formation.
