The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, indicative of a high stellar density. Moving outwards from the core, the luminosity gradually decreases, forming a diffuse halo. The overall color profile appears reddish-yellow, suggesting a population of older stars with relatively little ongoing star formation. There is a hint of asymmetry in the outer halo, potentially indicating a minor gravitational disturbance or past interaction.
