The galaxy presents a disturbed morphology, suggesting an ongoing or recent interaction. The primary body of the galaxy appears relatively smooth and elongated, potentially exhibiting a spheroidal shape. A distinct secondary component is observed, appearing smaller and slightly offset from the main body. The color distribution indicates variations across the galaxy, with a bluer hue in the more diffuse region and a tendency towards redder colors in the denser area. This may suggest areas of younger stars, while the redder colors can indicate older stars and dust. Given the irregular shape and color variations, star formation activity appears to be present, but not dominant. A tidal tail may be present, extending from one side of the galaxy. The features suggest a system undergoing a merging process, with the smaller component contributing to the overall disruption.
