The galaxy exhibits a distinct spiral morphology, characterized by well-defined arms. The arms appear tightly wound, wrapping around the central bulge. Star formation is evident within the arms, indicated by regions of bluish light, while the central bulge presents a yellowish hue. The galaxy appears to have a moderate bulge. There are no significant signs of any bar structure, and the overall structure suggests a spiral galaxy undergoing a minor disturbance, with no major interactions occurring at the present time. The image suggests that the galaxy is not perfectly symmetrical, potentially hinting at ongoing or past gravitational interactions.
