The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated luminosity, suggestive of a significant stellar population and potentially a supermassive black hole at its core. There's a noticeable lack of distinct spiral arms or prominent dust lanes. The light distribution appears spheroidal with a high degree of circularity. The overall color appears slightly redder in the central region, gradually transitioning to bluer hues at the periphery. The galaxy doesn't display any obvious signs of ongoing major mergers or strong tidal interactions with neighboring galaxies. Subtle asymmetries are present in the outer regions, possibly indicating minor disturbances or faint tidal features, but the dominant morphology is smooth and well-defined.
