The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be undergoing a significant merger or interaction, as evidenced by tidal features. The main body of the galaxy exhibits a nearly spheroidal shape with a smooth light distribution, suggesting a substantial bulge component. There are asymmetrical extensions or tails of light extending outward. These tails suggest recent or ongoing gravitational disruption, possibly due to a merger with a smaller galaxy, or close encounters with other galactic objects.

The color gradient of the galaxy suggests a mix of stellar populations. The central region appears slightly more yellow/red, indicating an older stellar population. The outer regions and tidal features appear bluer, suggesting ongoing or recent star formation in these areas.
