This galaxy exhibits a distinct spiral morphology, characterized by a well-defined disk. Two spiral arms are clearly visible. The arms appear loosely wound around a central bulge. The bulge itself appears relatively small. The disk shows evidence of ongoing star formation, with regions of bluer color interspersed throughout the spiral arms. There appears to be some form of gravitational disturbance occurring within the system, indicating possible recent or ongoing interaction with another galaxy. The overall structure is quite distinct.
