The galaxy appears to be a relatively smooth, elliptical type galaxy. It exhibits a centrally concentrated luminosity profile, with a gradual fading towards the outer edges. The galaxy presents an overall moderate ellipticity, leaning toward a cigar shape. There are no obvious signs of strong tidal disturbances or major merging events in progress, though a minor disturbance cannot be ruled out. Its color suggests a moderate amount of star formation. The galaxy has a substantial mass, and it’s likely experiencing a considerable amount of star formation, which could be triggered by a minor interaction. The galaxy appears to have an intermediate specific star formation rate.
