This galaxy exhibits a distorted morphology, suggesting an ongoing or recent interaction. The main body displays a moderately smooth appearance. A tidal tail or plume extending from one side indicates gravitational disturbance. The color gradient suggests some differences in stellar populations across the galaxy, with bluer regions possibly indicating areas of active star formation and a redder core. The overall shape deviates significantly from a regular elliptical or spiral structure, pointing toward a system undergoing dynamic change.
