The galaxy presents as a spiral type, exhibiting a disk-like structure. A central bulge dominates the core region, displaying a yellowish-orange hue, suggestive of an older stellar population. Fainter spiral arms emanate from the central bulge, exhibiting a bluer tint. The bluer color indicates the presence of younger, hotter stars and ongoing star formation within the arms. The spiral arms appear somewhat tightly wound around the bulge. The galaxy appears to be an average size, but not the largest or smallest of galaxies, with a slight ellipticity. No obvious signs of major merging activity or significant tidal disturbances are apparent, the morphology appears largely undisturbed. There is a weak, but visible bar across the galaxy.