The galaxy presents as a smooth, elliptical-like structure with a high degree of central concentration. The light distribution indicates a relatively old stellar population. Color gradients suggest a slightly bluer color in the outer regions compared to the core, which appears yellower. There is no apparent disk structure, spiral arms, or strong dust lane features visible. The galaxy exhibits a smooth light profile, with an overall rounded shape. There's no evidence of any major merger events or significant tidal disturbances in the immediate vicinity. The lack of distinct features points towards a system with little ongoing star formation.
