The galaxy appears to be undergoing a major merger event, based on the distorted morphology. It exhibits multiple distinct nuclei, suggesting the interaction of at least two significant galaxies. The shape is highly irregular, lacking a clear spiral or elliptical structure, instead showing signs of tidal tails or streams. The central region appears relatively smooth compared to the outer regions. The color distribution indicates varying stellar populations, with hints of recent or ongoing star formation in some areas, evidenced by a bluer hue. The system appears to be relatively compact.
