The galaxy presents as a moderately luminous, elliptical-like structure. Its overall morphology appears quite smooth with a high degree of central concentration. There is a distinct lack of spiral arm features or dust lanes visible. The color gradient suggests a population of older stars, exhibiting a yellowish-red hue, particularly towards the core. The galaxy does not show any apparent signs of recent or ongoing major mergers, though some minor asymmetry in its outer regions may indicate a past interaction or minor disturbance. The shape is largely round, with a slight elongation.
