The galaxy presents an elliptical morphology with a bright, concentrated nucleus. A bulge component is readily apparent, gradually fading into a more diffuse halo. The color profile indicates a generally older stellar population throughout the galaxy. There appears to be a weak disk extending beyond the bulge. The galaxy does not display any distinct spiral arms. It has a smooth overall appearance, showing no major disturbances or signs of on-going or recent merger events. There is no presence of dust lanes.
