This galaxy exhibits a prominent disk structure with well-defined spiral arms. The arms appear relatively tightly wound, suggesting a grand design spiral galaxy morphology. There is evidence of active star formation within the arms, indicated by the presence of blue regions, likely representing populations of hot, young stars. The central bulge is moderately sized and appears yellowish, indicating an older stellar population. The galaxy is viewed nearly face-on, allowing for clear observation of its spiral structure. There is a subtle bar-like feature bisecting the central region. Overall, the galaxy appears to be a relatively massive and actively star-forming system. There is a possible minor disturbance visible in the overall morphology.
