The galaxy appears to be a relatively smooth, elliptical-type galaxy. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in surface brightness outwards. There is a bright, unresolved core, surrounded by a diffuse halo. The galaxy exhibits a yellowish-red hue, indicating a population of older stars, with little to no active star formation observed in this image. The overall shape is generally round, and there is no visible evidence of any major tidal disturbances or ongoing mergers. The light is evenly distributed and the overall structure suggests that this galaxy has undergone significant dynamical relaxation.
