The galaxy presents as a somewhat elliptical structure with a smooth, centrally concentrated luminosity profile. The core region exhibits a bright, yellow-white hue, suggestive of a relatively old stellar population. Extending outwards from the core, a fainter, more diffuse halo is observed. There is a hint of a disk-like structure. There appears to be a plume of gas and dust or tidal streamer extending away from the main body of the galaxy, potentially indicating a past or ongoing interaction. The overall color suggests a galaxy with a substantial population of older stars and a comparatively low rate of current star formation.
