This galaxy appears to be undergoing a major merger. There are two distinct, bright nuclei visible, suggesting a late-stage interaction between two galaxies. The overall shape is highly disturbed and irregular. The color distribution indicates a mix of stellar populations; the prominent redder components potentially indicate older stars or significant dust obscuration, while the fainter surrounding bluish-green hue points toward a possible presence of ongoing star formation, likely triggered by the merger event. There appears to be a tidal bridge or tail extending from the main body of the galaxy, further evidence of a disruptive gravitational interaction. The morphology is far from elliptical or disk-like. The estimated size indicates that this is a relatively large galaxy.
