The galaxy presents a disk-like morphology, viewed at an angle that is somewhat close to face-on. A central bulge region is evident, appearing as a concentration of light in the galaxy's core. Faint spiral arm structures emanate from the central bulge and extend outwards. The spiral arms are somewhat tightly wound. There are about 3 spiral arms that can be distinguished. The galaxy is relatively large, with a somewhat elliptical shape overall. There is a slight blue tinge to some of the spiral arm regions. No signs of any type of galaxy mergers can be observed. There appears to be a bar structure within the galaxy, though it is difficult to say whether it is weak or strong from the image.
