The galaxy presents as a diffuse, relatively smooth, and rounded structure. There is a bright central concentration, possibly indicative of an active galactic nucleus or a dense stellar population in the galactic bulge. The overall color appears reddish-yellow, which could suggest a population of older stars or significant dust obscuration. There appears to be some disruption to the overall smooth structure, with hints of tidal features or interactions with a close companion. There are suggestions of a distorted or warped disk structure in the galaxy, further supporting the possibility of past or ongoing gravitational interactions. Faint, diffuse light extends outwards from the central region.
