The galaxy presents an elliptical morphology, appearing largely smooth in structure with minimal discernible features such as spiral arms or prominent dust lanes. Its shape is generally rounded, with a slight deviation towards an elongated form. The galaxy exhibits a color gradient, transitioning from a bluish central region to a redder halo. This suggests ongoing star formation activity concentrated towards the core, with older stellar populations dominating the outskirts. There is no strong evidence of a major merger event, though there is a faint asymmetrical feature in the halo that could be an indication of a minor disturbance or past interaction.
