The galaxy appears as a relatively smooth, centrally concentrated object. It presents a largely elliptical morphology with high degree of roundness. There are no clear indications of spiral arm structure or a prominent central bulge. The galaxy appears to be a single, relatively undisturbed system, showing no evidence of major mergers or significant tidal disturbances. Subtle indications of minor disturbances could be present. The galaxy is predominantly bluish in color, suggestive of ongoing, but not necessarily vigorous, star formation. This observation is derived from comparing the green, red and z magnitudes. The galaxy displays a diffuse, extended halo.
