This galaxy exhibits a clear spiral structure. The spiral arms are tightly wound, originating from a central bulge. The bulge appears relatively small in proportion to the overall disk size. The color of the galaxy shifts from yellowish-white in the center to bluish hues in the outer spiral arms, indicative of a population of younger, hotter stars in the arms. The disk is not perfectly edge-on, presenting a tilted view that allows observation of the spiral arm structure. There is no obvious sign of major interaction or merging with another galaxy. A faint bar appears to be present.