The galaxy exhibits a distinct spiral morphology. Its disk is observed face-on, presenting a clear view of its spiral structure. Multiple spiral arms emanate from the central region. The arms appear tightly wound, displaying a flocculent structure with several branching and interwoven segments. The central bulge appears small in relation to the disk size. Patches of blue suggest recent or ongoing star formation within the spiral arms. There is no evidence of a significant bar structure crossing the center of the galaxy. The overall structure appears undisturbed, with no apparent signs of major interactions or mergers.