The galaxy appears as a largely featureless spheroid. It exhibits a bright, concentrated core region that gradually diffuses outwards into a more extended halo. There is subtle color variation present. The central core appears more reddish, possibly indicative of an older stellar population or dust obscuration. The outer halo shows hints of bluer hues, which could suggest younger stars and ongoing star formation. Overall, the galaxy appears relatively smooth and undisturbed, showing no prominent spiral arms or signs of a recent major merger event. It has an apparent elliptical shape. The galaxy's light distribution is centrally concentrated, indicative of a galaxy dominated by a large bulge. There is a distinct fading of light toward the edges of the galaxy.
