The galaxy presents as a generally smooth, elliptical structure, with a high degree of central concentration. The primary light emission is concentrated in a round core. There is a hint of a slightly more diffuse region extending outwards, with a slight elongation to the left. Color gradients suggest a redder central bulge and a slightly bluer, albeit faint, outer disk, hinting at possible recent star formation. The galaxy appears relatively undisturbed, showing no strong evidence of a major ongoing merger.
