The galaxy presents a distinct spiral morphology. Tightly wound spiral arms emanate from a moderate-sized central bulge. There appears to be a bar-like structure spanning across the bulge, though it is not strongly defined. The arms display a generally cohesive structure, dominated by two major arms. The overall color of the galaxy suggests ongoing star formation, particularly within the spiral arms, and a likely relatively young stellar population in the disk. The central bulge exhibits a yellowish hue, possibly indicating an older stellar population with less active star formation. The presence of some irregularities in the arm structure may point toward minor gravitational disturbances. Overall, the galaxy appears as a moderately massive spiral galaxy undergoing active star formation.
