The galaxy presents as a spiral type, with a moderately inclined disk. The spiral arms are quite well defined, with a tightly wound morphology. There appears to be a central bulge, although it is not highly pronounced. The overall color suggests ongoing star formation within the galaxy. There may be some indications of a bar structure in the central region, though this is not definitively observed. The disk appears relatively undisturbed, showing no major signs of recent mergers or significant interactions.