The galaxy presents as a disk galaxy, viewed at a slight inclination. There is a prominent central bulge exhibiting a smooth, concentrated luminosity profile. The disk shows indications of spiral arm structure, though it is somewhat flocculent. Two spiral arms appear to emanate from the central bulge, and are not tightly wound. The overall color of the galaxy is consistent with a mix of stellar populations, with some regions exhibiting bluer colors indicative of more recent star formation.
