The galaxy presents as a centrally concentrated elliptical-like structure. The core exhibits a yellowish-white hue, suggesting a dominant population of older stars. The overall shape is moderately elongated, not perfectly spherical, and is relatively smooth in appearance, showing limited signs of spiral arms or significant dust lanes. Some very faint hints of extended features around the central bulge might be present, but these are quite indistinct. There is no clear evidence of any major ongoing merger or tidal disruption events, though a slight asymmetry might suggest a minor past interaction.
