The galaxy presents a distinct spiral morphology. It is observed at a slight inclination, permitting partial visualization of its spiral structure. The spiral arms are tightly wound around a moderately sized bulge. While somewhat indistinct, the spiral arm count appears to be three. No strong bar feature is discernible. The overall structure of the galaxy exhibits no obvious signs of major disturbance or interaction with other galaxies. The central bulge is bright, and the spiral arms are relatively faint and smooth. 
