The galaxy presents as a system with a dominant central spheroid component. The primary component exhibits a smooth light distribution, with a concentrated core and a gradual decrease in surface brightness outwards. The overall color appears yellowish-white, potentially indicative of an older stellar population. The galaxy's shape is somewhere between round and slightly elliptical. There is an apparent disturbance on the right side of the galaxy, perhaps indicating the presence of a companion galaxy or tidal interaction, which could be a minor disturbance or a more significant merger event. There are also some redder regions surrounding the galaxy which could be related to star formation regions.
