The galaxy presents as a relatively bright, face-on spiral. There is a prominent central bulge exhibiting a yellowish hue, suggesting an older stellar population. Fainter spiral arms emanate from the bulge. The arms appear somewhat diffuse and patchy. A disk is present, but is not as distinct as some other spiral galaxies. There are no obvious signs of a major merger or strong tidal disturbances, though some minor irregularities could be indicative of past interactions or accretion events. Overall, the galaxy appears relatively normal in morphology for its type.