The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated luminosity with a yellowish hue, suggestive of an older stellar population. A faint, diffuse halo of bluish light surrounds the core, indicating the presence of some younger, hotter stars. The overall structure appears relatively undisturbed, lacking any obvious signs of recent major mergers or tidal interactions. There might be a very subtle disk like structure, but it is difficult to tell from the image, and could just be an artifact of light distribution. Overall, the galaxy seems to be relatively quiescent in terms of star formation activity.
