The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright core region, surrounded by a more diffuse halo. The color profile of the galaxy shows a redder hue in the central region, indicating an older stellar population, with a bluer halo, likely caused by younger stars. There are no obvious spiral arms or dust lanes visible. There are minor signs of tidal disturbance suggesting a small merger event in the past. The overall appearance suggests a galaxy that is relatively evolved.
