The galaxy presents a generally elliptical morphology with a high degree of central concentration. The core is luminous, exhibiting a yellowish-white color indicative of an older stellar population. The outer regions fade gradually and show a hint of a flattened disk-like structure. There is a slight color gradient from the core outwards, with the outer regions appearing slightly bluer, suggesting the presence of some younger stars. The overall appearance is relatively smooth, without prominent spiral arms or significant dust lanes. There's also a hint of a slight asymmetry or perturbation in the galaxy's morphology, suggesting a possible past interaction or minor disturbance.