The galaxy presents as a relatively compact, elliptical structure with a smooth, diffuse light distribution. It exhibits a largely featureless morphology, lacking prominent spiral arms or a distinct bar structure. The galaxy's shape is generally round. There are no indications of major ongoing merger activity or significant tidal disturbances, though the possibility of minor disturbances cannot be entirely excluded. The overall color suggests a population of older stars, with a tendency towards redder hues throughout the galaxy body. The galaxy's apparent size is small, indicative of its considerable distance. It is a substantial galaxy, likely containing a high mass. Star formation appears to be low within this galaxy.
