The galaxy presents a relatively smooth, rounded morphology. It appears to have a dual core or nucleus, suggesting a possible interaction or merger event. There is some evidence of a minor disturbance in the overall structure. The galaxy exhibits a color gradient, with a central region displaying yellower hues, potentially indicative of an older stellar population, surrounded by bluer regions. Based on its apparent smoothness and roundness, this galaxy may be an elliptical galaxy, potentially undergoing a merger. Star formation appears to be occurring, but at a moderate rate.
