The galaxy presents as an elliptical-like structure with a slight elongation. A bright, concentrated core region dominates the central area, indicative of a substantial stellar population. The light profile decreases gradually moving outward from the core. A faint disk is detected surrounding the core, with subtle hints of spiral arm structures. There is no significant dust lane apparent upon visual inspection of the image. The galaxy appears to be relatively isolated. The overall color of the galaxy is yellowish in the center transitioning to a bluish tint in the outer regions, suggesting a mix of older stellar populations in the core and younger, bluer stars within the disk.
