The galaxy presents a somewhat elliptical morphology, though nearing a circular shape, which is indicative of a late-type or spiral galaxy viewed face-on. A bulge is present, and it dominates the overall light distribution. The light distribution within the bulge appears relatively smooth and centrally concentrated. The outer regions of the galaxy appear fainter and less well-defined, with a general color that suggests the presence of older stellar populations. There is no readily apparent spiral arm structure or significant dust lanes visible in the image.
