The galaxy appears to be an elliptical galaxy. It presents as a relatively smooth, concentrated object with a somewhat round appearance. Some degree of disturbance is suspected with an unclear feature in the top. No pronounced spiral arms or disk-like structures are observed in the image. The galaxy exhibits a noticeable color gradient, with a bluer core transitioning to redder outskirts, suggestive of a varied stellar population. This galaxy is estimated to be a moderately sized with an active, but slowing rate of star formation. The overall morphology indicates a system that is likely undergoing, or recently underwent, a merger event.
