The galaxy appears to be undergoing a significant merger event. It displays an irregular morphology, with indications of tidal disruption. A luminous bridge of material is visible, connecting what appear to be two distinct galactic cores or high density regions. These regions exhibit a reddish-orange hue, suggesting older stellar populations or significant dust obscuration. There is a bluer region, potentially indicative of ongoing star formation, associated with one of the merging components and stretching along an arc shape of the galaxy. The overall structure is complex and lacks a well-defined spiral or elliptical shape.
