The galaxy presents as a spiral galaxy with a prominent central bulge. Two spiral arms are clearly visible, winding outwards from the core. The arms appear somewhat flocculent, with regions of enhanced brightness suggesting active star formation. The core is relatively bright and concentrated, potentially indicating a substantial population of older stars or the presence of an active galactic nucleus. There's a slight asymmetry in the distribution of light within the disk, which could be caused by interactions with other galaxies or internal processes like a bar structure. The galaxy's overall shape appears to be close to face-on.
