The galaxy presents as an elliptical structure with a smooth, concentrated light distribution. There is a prominent central bulge exhibiting a bright, yellowish-white hue suggesting a population of older stars. The overall form is slightly elongated, deviating marginally from a perfect sphere. Faint extensions are seen around the central region, but there is no indication of spiral arms or other disk-like features. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. There are hints of bluer light in the outer edges, potentially indicating some amount of ongoing star formation activity, though at a low level. Overall, the galaxy appears to be a fairly massive, relatively evolved system with a dominant spheroidal component.
