The galaxy appears as a relatively smooth, elliptical-like structure. It displays a centrally concentrated brightness, gradually decreasing in intensity outwards. The overall shape is mostly round. There are some indications of potential minor disturbances or irregularities in the outer regions, hinting at possible tidal interactions or past merger events, though the dominant impression is one of a well-defined, settled morphology. The color profile suggests a population of older stars dominating the stellar content, with a redder hue in the core region. The galaxy appears fairly massive, typical of galaxies residing within galaxy groups or clusters. Star formation appears to be either low or absent.
