This galaxy presents a disk-like structure, observed at a significant inclination. It exhibits prominent spiral arms. The central bulge appears relatively small compared to the overall disk size and has a yellow hue, suggesting an older stellar population. The spiral arms appear tightly wound, and are blue in color, indicating active star formation. The galaxy is likely undergoing a process of star formation, with a moderate star formation rate. There is no strong evidence of any major merging events, though some minor disturbances may be present. A bar structure appears to exist in the center. The image is somewhat blurred, impacting the precision of morphological analysis.
