The galaxy appears to be undergoing a merger event, with two distinct, relatively smooth components visible. The components exhibit a slightly elliptical morphology. There are noticeable tidal features and minor disturbances, likely stemming from the gravitational interaction. The overall color is yellowish and there are hints of redder regions concentrated in the core, possibly indicating older stellar populations and dust obscuration. The galaxy has a substantial mass, evidenced by the scale of the merging event. Star formation may be subdued due to the advanced stage of the merger.
