The galaxy presents as a concentrated, centrally-brightened system. The light distribution appears mostly smooth, with a slightly elliptical morphology. There is a notable asymmetry present in the form of a secondary concentration of light located off-center, possibly indicating a minor disturbance. The colors are indicative of an aging stellar population and minimal ongoing star formation. The galaxy's redder color suggests it has a substantial mass and minimal star formation. It's possible this system is in the process of merging with a smaller galaxy.
