The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its light profile appears relatively uniform, lacking distinct spiral arm structures or prominent dust lanes. The core exhibits a high surface brightness, suggesting a dense stellar population or the presence of an active galactic nucleus. Fainter, diffuse light extends outwards from the core, gradually decreasing in intensity. There is a subtle color gradient visible, with the central region appearing slightly yellower compared to the outer regions which appear more reddish. The overall structure lacks any signs of major disturbances or ongoing mergers, implying a relatively relaxed dynamical state.
