The galaxy presents a generally smooth, elliptical morphology with a notable central bulge. The light distribution appears concentrated towards the core, diminishing gradually outwards. There is some indication of a slight disk-like structure, though features are not prominent. The galaxy exhibits a color gradient, shifting from a reddish-hue in the core to a bluer-hue in the outer regions. No obvious signs of major disturbances like tidal tails or strong asymmetry are observed, though minor irregularities are visible and may indicate minor disturbances, such as a potential ongoing or recent minor merger.
