The galaxy exhibits a clear spiral structure. The arms are relatively tightly wound. Evidence of flocculent spiral arms can be seen. The central bulge is small. The disk is oriented approximately face-on. There is no obvious bar structure present. No signs of major mergers are readily apparent, but some disturbances or irregular structures hint at possible minor interactions or past mergers. The galaxy's color suggests the presence of both older stellar populations, as indicated by the reddish hues, and younger, bluer stars, particularly in the spiral arms. The galaxy possesses a general blue hue throughout. 
