The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, tending towards an intermediate shape between round and elongated. There is a suggestion of a minor disturbance in the galaxy's structure. The galaxy displays a central, concentrated region of bluer light, possibly indicative of ongoing star formation. This central region fades outwards into a more diffuse halo, which appears redder in hue. The redder color is likely due to an older stellar population.
