The galaxy appears as a relatively smooth, elliptical-shaped object with a concentrated central bulge. The light distribution is generally consistent and symmetrical around the center. There may be an indication of faint, extended emission surrounding the primary body of the galaxy, but no distinct spiral arms or other disk-like features are readily apparent. The color profile suggests a population of older stars, indicated by the redder hue, with a slight shift toward bluer colors in some areas. No significant tidal features or signs of recent major mergers are discernible. There is no obvious dust lane or any internal structure. The overall impression is that of a mature, early-type galaxy.
