This galaxy exhibits a discernible spiral structure, although the arms are somewhat flocculent and lack sharp definition. There is evidence of a central bulge, but it appears relatively small and less prominent compared to the overall disk. The spiral arms seem to initiate close to the center of the galaxy. Some regions appear potentially distorted, possibly indicative of minor gravitational interaction or recent merging activity, but its overall structure is still intact. The winding of the spiral arms appears to be predominantly tight to medium. The galaxy presents a rich array of features, suggesting ongoing star formation within the disk and spiral arms.
