The galaxy presents as a spiral type, with a notable disk structure. It is not viewed perfectly edge-on, but at a slight angle. The spiral arms are tightly wound and are quite pronounced. The central bulge is relatively small and unobtrusive. There appears to be no strong bar feature bisecting the galaxy's core, but the arms are very close together. No major disturbances or clear signs of ongoing or recent mergers with other galaxies are immediately apparent, though minor irregularities in the arm structure cannot be ruled out. The spiral arms are tightly wound. The color of the galaxy's arms indicates active star formation.
