The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-circular morphology. The light distribution suggests a dominant spheroidal component, possibly with a small disk. There is a central concentration of light with a radial falloff. The galaxy's color is somewhat yellowish, possibly indicating an older stellar population with little active star formation. There are no readily discernible tidal features or signs of recent major merger activity. A minor disturbance cannot be ruled out, but it is not immediately obvious from the data.
