The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits high luminosity, indicating a dense concentration of stars, likely older populations given the yellow-red color. A fainter, diffuse halo surrounds the core, gradually fading into the background sky. The overall structure shows a slight elongation, deviating somewhat from a perfect circular form. There is little indication of spiral arm structures or significant dust lanes. Minor asymmetries might be present, possibly suggesting a past interaction or minor disturbance, though the dominant impression is one of relative quiescence.
