The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears dominated by a bulge component, exhibiting an elliptical morphology. The galaxy appears elongated, but not dramatically so. Faint outer regions suggest a possible disk component, however the disk is ill-defined. There is no strong evidence of spiral arms. The overall color is yellowish-orange, suggesting a population of older stars. The absence of strong blue colors indicates a relatively low rate of ongoing star formation. No strong tidal features or signs of recent major mergers are apparent, although a possible minor disturbance cannot be ruled out.
