The galaxy presents as a centrally concentrated object, likely an elliptical galaxy. It exhibits a smooth, relatively featureless morphology, lacking prominent spiral arms or distinct disk structures. The light is dominated by a yellow-red hue, suggestive of an older stellar population. The galaxy appears quite rounded, with a high degree of rotational symmetry. There appears to be some evidence of a minor disturbance on the side, perhaps a tidal tail or minor merger remnant. The galaxy has a moderate degree of star formation activity. It is a relatively massive galaxy.
