The galaxy presents as a largely featureless, elliptical object. It exhibits a smooth, concentrated light profile, with the highest intensity at the center, gradually decreasing outward. There is no discernible spiral arm structure or dust lane features. The galaxy appears largely spheroidal in shape, with a high degree of roundness. No major signs of ongoing or recent merger activity are immediately apparent, although minor disturbances cannot be ruled out based on visual inspection alone. The color indices suggest a population of older stars, exhibiting higher emission in the redder bands.
