The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The dominant color appears to be reddish, with a slight gradient towards a yellower hue at the core, suggesting a population of older stars. The outer regions exhibit a fainter, diffuse halo extending beyond the central body. A subtle hint of a disc structure is observable, although the overall morphology is overwhelmingly dominated by the elliptical component. There are no visible signs of strong tidal interactions or major mergers. The galaxy exhibits a weak star formation rate as suggested by its color.
