The galaxy presents an elliptical morphology, with a smooth light distribution, suggesting an evolved stellar population. Its color gradient indicates a concentration of older, redder stars towards the center, with a faint, diffuse blueish component that extends from the center. No distinct spiral arms or other prominent features are discernible; however, some minor disturbances appear to be present. The galaxy is a relatively rounded shape. Based on the light profile and colour distribution, the galaxy seems to be undergoing very little star formation. Given the estimated size and luminosity, this is a relatively massive galaxy.
