The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high degree of luminosity, suggesting a concentration of older stellar populations. The galaxy does not display any prominent spiral arm structures or dust lanes. There may be a slight asymmetry in the outer halo, with some minor perturbations or tidal features indicating a possible past interaction or minor merger event, but further high resolution images are required to confirm this. The overall color appears redder, consistent with a passively evolving system.
