The galaxy presents as a relatively smooth, elliptical-like structure with a bright central bulge. It exhibits a somewhat elongated shape, suggesting it is not perfectly spherical. There is a lack of discernible spiral arm structures or strong dust lanes. The light distribution appears concentrated towards the center, gradually fading outwards. There is a hint of a disk-like component, though it is quite subtle. No obvious signs of major mergers or significant tidal disturbances are visible. The overall color suggests a stellar population that is possibly evolved, with less ongoing star formation.
