The galaxy presents as a spiral type, displaying well-defined spiral arms that originate close to the bright central bulge. The arms exhibit a tightly wound structure. The galaxy is face-on, providing a clear view of its spiral morphology. The central bulge appears relatively bright and concentrated. The disk is resolved, with blue regions indicative of active star formation within the spiral arms, and some areas appear to indicate the presence of dust. There is no obvious, major merging activity taking place, although minor disturbances cannot be ruled out. The galaxy appears relatively isolated.
