The galaxy presents as a face-on spiral galaxy with a moderate bulge size relative to the disk. The spiral arms are quite prominent, although the structure is not fully resolved. It is difficult to discern the exact number of arms, but there may be two major arms. The arms appear to be moderately tightly wound. There is no clear indication of a bar structure. The light distribution suggests the galaxy is not perfectly smooth, instead exhibiting clear signs of star formation within the disk. The core of the galaxy is notably bright, indicating either a high concentration of stars, or potentially low-level AGN activity. There is no obvious evidence of tidal features, or a major ongoing merger, though a minor disturbance within the disk cannot be ruled out.
