The galaxy presents as a relatively smooth, elliptical-like structure, though it's not perfectly spherical. It appears to be more lenticular in shape with a slight elongation. There is some suggestion of a faint, broad disk-like structure, but this is subtle. The galaxy's light is concentrated toward the center, showing a bright core. Color gradients indicate a predominantly older stellar population, with a redder hue, though there is some suggestion of bluer regions indicating more recent star formation. There may be a very slight disturbance in its overall form, hinting at a possible past interaction or minor merger event.
