This galaxy presents as a luminous elliptical structure, displaying a smooth, concentrated morphology. The central bulge exhibits a bright, yellowish-white hue, suggesting a population of older, evolved stars. Moving outwards from the core, the luminosity gradually decreases, transitioning to a more diffuse, reddish-yellow halo. There is a slight elongation, indicating a deviation from a perfectly spherical shape. Faint hints of a surrounding envelope are visible, though no distinct spiral arms or prominent dust lanes are discernible in this image, nor any signs of major interactions or mergers. A minor asymmetry is observed in the outer halo, suggesting a possible past interaction or tidal disturbance.
