The galaxy appears to be an elliptical galaxy, exhibiting a smooth, somewhat spheroidal morphology with a concentrated central bulge. The light distribution indicates a centrally concentrated luminosity profile. The core region is dominated by a yellowish-white hue, likely indicating an older stellar population. The outer regions appear to be less luminous, gradually fading into the background sky. There is a hint of bluer light in the outer regions, suggesting the presence of some younger, though not particularly prominent, stars. There are some features indicating this galaxy is in the process of merging. I cannot tell the exact number of mergers it has undergone or is undergoing. No strong spiral arm features or distinct dust lanes are visible. There also appears to be a degree of activity within the galaxy, with an estimated star formation rate that is a bit higher.
