The galaxy appears to be undergoing a significant merger event, likely between two or more galaxies of comparable mass. The primary body exhibits a generally elliptical morphology but displays considerable tidal distortion, presenting an irregular and disturbed form. There is evidence of significant tidal tails or bridges extending outwards, indicating strong gravitational interaction with another galaxy.

The color profile suggests a population of primarily older stars, giving it a yellowish-red hue, indicating suppressed star formation. However, there are areas of bluer color as well, suggesting on-going star formation, likely triggered by the merger.
