The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge that transitions into a more diffuse halo. The color profile of the galaxy indicates a primarily older stellar population, with a yellow-red hue prominent throughout the main body of the galaxy. The central bulge appears to be the brightest and most concentrated region, potentially indicating a high density of stars. There is a hint of a faint disk-like structure surrounding the bulge, characterized by a slightly bluer tinge, although the disk is not well-defined. There is no evidence of strong spiral arm features, active star formation regions, or a significant amount of dust obscuration in this galaxy. The overall impression is of a galaxy that is fairly evolved and quiescent. There do not appear to be any signs of any recent or ongoing mergers.
