This galaxy appears to be a relatively smooth, elliptical galaxy. It presents a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades outwards. There is little evidence of distinct spiral arms or significant dust lanes within the galaxy. The galaxy appears to be primarily spheroid in shape. The color gradients suggest that the core may be composed of older stellar populations, while the outer regions may contain a small amount of younger stars. There are no obvious signs of any major ongoing merger events or tidal disturbances.
