The galaxy presents as a singular, smooth object with an elliptical morphology. There is a distinct central bulge that appears relatively bright and concentrated, with a yellowish hue, suggesting an older stellar population. The overall light distribution smoothly decreases from the center outwards, and the edges are diffuse and without any apparent spiral arm structures or significant dust lanes. The galaxy appears to be relatively isolated and does not show obvious signs of tidal disturbances or ongoing mergers. The object exhibits a slight elongation, neither perfectly circular nor highly flattened.
