The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, presenting a rounded appearance. The color profile shows a redder hue overall, especially toward the center, suggesting an older stellar population. There is no obvious disk structure. Some minor disturbances are apparent as the galaxy exhibits a more irregular shape. The galaxy is undergoing a merging event with another galaxy. The mass estimate is indicative of a substantial galaxy. The galaxy's estimated star formation rate is quite low.
