The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. The arms appear tightly wound around a central bulge, though precise arm counts are difficult to ascertain from this image. The bulge itself seems moderately sized relative to the overall disk of the galaxy. The galaxy's disk is viewed face-on and does not appear edge-on. The overall color suggests active star formation within the spiral arms, with bluer regions interspersed amongst yellower regions. There is no obvious strong central bar structure, but a subtle bar may be present. No major merging activity is immediately apparent, however, slight disturbances in the arms cannot be ruled out.
