The galaxy presents as a spiral galaxy, displaying a distinct disk structure. There is evidence of spiral arms originating from a central bulge. These arms appear somewhat tightly wound. The overall color suggests a relatively evolved stellar population, though subtle variations within the arms hint at on-going star formation. The central bulge appears moderately sized and bright. The galaxy does not appear to be undergoing any major mergers, though minor disturbances or tidal features cannot be ruled out. There appears to be a bar-like structure that may or may not be present within the structure. The overall shape of the galaxy is symmetrical.
