This galaxy presents as a moderately bright, disk-shaped object with a noticeable bulge. The disk appears relatively smooth. There is a subtle suggestion of spiral arm structure. The central bulge region exhibits a more concentrated brightness. The outer edges of the disk show a slight fuzziness, possibly indicative of ongoing star formation or tidal interactions. Based on its morphology, it may be an intermediate spiral galaxy of type Sa, Sb, or Sc but with a very low inclination angle. There is a chance the galaxy is undergoing a minor merger.
