The galaxy presents as an elliptical-like morphology, with a noticeable elongation along its major axis. The central region is characterized by a bright, concentrated nucleus, exhibiting a yellowish-white hue suggestive of an older stellar population. Moving outwards from the core, the galaxy displays a smoother, less structured appearance, with a gradual decrease in surface brightness. The overall color gradient shifts towards bluer tones in the outer regions. A subtle asymmetry appears on one side of the galaxy, possibly indicating tidal disturbances or interactions with a smaller companion, or areas of increased star formation. Overall, the galaxy appears relatively isolated within its environment, although higher resolution imaging is necessary to detect smaller, fainter satellite galaxies.
