This galaxy presents as a fairly smooth, elliptical-like structure, elongated along one axis. The color appears to be a yellowish-white, suggesting an older stellar population with fewer young, hot stars. The overall light distribution seems concentrated towards the center, with a gradual decrease in brightness towards the outer edges. There are no distinct spiral arms or prominent dust lanes visible. The galaxy appears relatively undisturbed with no signs of major mergers or tidal distortions based on the lack of visual disruption. There appears to be an indication of minor disturbance within the galaxy, although it is not obvious.
