The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a radial decrease in luminosity. The galaxy's color appears somewhat redder, potentially indicative of an older stellar population. The light distribution suggests a slight elongation. Faint, extended halo-like structures are possibly present but difficult to discern definitively given the image quality. No distinct spiral arms or significant dust lanes are apparent. The galaxy appears relatively undisturbed, without obvious signs of a recent major merger or strong tidal interactions.
