The galaxy exhibits a generally smooth morphology, with a slight elongation in its overall shape, appearing somewhat cigar-shaped. The light distribution suggests that this is likely an elliptical galaxy. The concentration of light is highest towards the center, gradually decreasing towards the outer regions. The galaxy has a redder color, indicating an older stellar population and lower levels of on-going star formation. There are no prominent spiral arms or distinct features easily discernible, suggesting that major mergers are unlikely. There may be some signs of minor disturbances, however, the overall structure is relatively undisturbed, and the galaxy is likely in a relatively quiescent state. The size of the galaxy indicates that it is a relatively massive system.
