The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form appears elliptical or lenticular, with minimal discernible spiral structure. The light profile exhibits a strong central bulge, characterized by a yellowish-orange hue, suggesting a dominant population of older stars. This color shifts subtly outwards. There is little evidence of active star formation regions or prominent dust lanes based on this image, which could be the reason for the lack of blue/purple hues. The galaxy's periphery fades smoothly into the background, showing no clear signs of tidal interactions or major disturbances from mergers. There is a small amount of asymmetry in the halo.
