This galaxy exhibits a prominent spiral structure. The spiral arms are loosely wound, extending outwards from a central bulge. The bulge appears relatively small, exhibiting a moderate concentration of light. Within the spiral arms, there are noticeable regions of star formation, indicated by a bluish hue, suggesting the presence of young, hot stars. The overall color of the galaxy is slightly blue-shifted, indicating active star formation. A faint bar-like structure may be present across the center of the galaxy. There appear to be disturbances to the galaxy, suggesting an active history that may include interactions with other galaxies. The galaxy is disk-dominated.
