The galaxy presents as a face-on spiral with a notable disk structure. Spiral arms are evident, exhibiting a winding pattern that transitions from moderately to loosely wound as they extend outwards from the central region. A bulge is visible, appearing to be of moderate size relative to the disk. There is no apparent bar structure. Evidence suggests the presence of two major spiral arms that are easily discernable. The galaxy shows little indication of major disturbances or mergers. The overall color suggests moderate star formation activity.
