The galaxy presents as a disk galaxy with a prominent central bulge. The disk exhibits a non-uniform color distribution, suggesting ongoing star formation within the spiral arms. These arms appear somewhat loosely wound and are not sharply defined, giving the galaxy a flocculent appearance. A bar structure is visible in the central region, extending across a significant portion of the bulge. The color of the bulge is generally redder than the disk, indicative of an older stellar population. There is a possibility of minor tidal disturbances, as the galaxy's overall shape is not perfectly symmetric. It has an apparent edge-on profile.
