The galaxy presents as a relatively smooth, elliptical morphology. There appears to be little to no organized spiral structure or significant dust lanes visible. The light is highly concentrated toward the center of the galaxy, with a somewhat diffuse halo extending outwards. The color gradient is subtle, shifting from a yellowish-white core to a slightly greener periphery, which could indicate some low-level star formation, although the dominance of yellow suggests a primarily older stellar population. The shape is nearly circular, with only a slight deviation from perfect roundness. There are no obvious signs of major mergers or tidal disturbances in the immediate vicinity. The smooth and concentrated light profile suggests this galaxy is likely an evolved system.
