The galaxy presents as a generally smooth, elliptical object with a dominant central bulge. There is little to no evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a slight elongation, appearing more oblate than perfectly spherical. The color gradient suggests an older stellar population, with a reddish-yellow hue concentrated in the central region, indicating a population of evolved stars. The outer regions of the galaxy appear slightly bluer and more diffuse, possibly indicating some ongoing, albeit limited, star formation. There is no obvious indication of a major ongoing merger, though a subtle asymmetry on one side might suggest a past interaction or minor disturbance.
