The galaxy presents as a relatively face-on spiral with a clearly defined central bulge exhibiting a yellowish-white hue. The spiral arms are tightly wound and blue, indicating active star formation. There appear to be multiple arms, greater than four, extending outward from the central region. The galaxy is slightly elliptical in shape, with a high degree of circularity. There are a few localized, brighter regions of blue within the spiral arms, likely HII regions or star clusters. Overall, the galaxy displays a classical spiral morphology. There appears to be no significant dust lane obscuring the central bulge, and no evidence of major mergers or tidal distortions.
