The galaxy appears to be undergoing a merger. The primary galaxy exhibits a central bulge with a surrounding, disturbed disk structure. There are visible tidal features, suggestive of gravitational interaction. Specifically, a faint tail-like extension is observed, extending from the main body. The morphology is disturbed, with asymmetries in the light distribution. The color profile suggests ongoing star formation in certain regions, particularly within the disk, exhibiting bluer hues compared to the central bulge. Some diffuse light is visible around the galaxy.
