The galaxy presents a largely smooth, elliptical morphology. The light profile appears concentrated towards the center, which exhibits the brightest intensity. Proceeding outward, the intensity gradually diminishes without any prominent spiral arm structures or distinct features. There is a slight elongation observable, with the galaxy's shape being neither perfectly circular, nor particularly flattened. Subtle disturbances in the morphology suggest a possible minor interaction, but no major merger or strong tidal distortions are apparent. Color gradients across the galaxy are visible, with the central region appearing more yellow in hue and the outer regions having a bluish tint, implying older stellar populations centrally and younger populations perhaps in the outskirts. The galaxy shows a well-defined structure with minimal distortion.
