The galaxy presents as a single, consolidated object with a smooth, elliptical morphology. A pronounced central bulge is evident, exhibiting a concentrated luminosity profile. The galaxy's color appears generally redder in the central regions, potentially indicative of an older stellar population or significant dust obscuration. The outer regions are less distinct, fading gradually into the background sky. There are no clear signs of spiral arms or significant disk-like structures. The object is relatively undisturbed, showing no major tidal features or signs of ongoing mergers. The overall structure suggests that the galaxy is a relatively evolved system.
