The galaxy presents as a somewhat face-on spiral, exhibiting distinct spiral arm structure. These arms are relatively tightly wound and possess a slightly flocculent appearance. There appears to be some degree of active star formation occurring within these arms, suggested by the bluer color. The central bulge is moderately sized, and not particularly prominent, with no noticeable bar structure. There might be a small amount of tidal disturbance, and there is no apparent sign of an on-going merger with another galaxy. It is relatively small in size and displays a moderately low surface brightness. The disk of the galaxy is not observed edge-on and the majority of the light is contained within the galaxy itself, rather than any sort of extended halo.
