The galaxy appears as a centrally concentrated light source, with a smooth, elliptical morphology. There is a noticeable lack of distinct spiral arm structure or prominent dust lanes. The galaxy exhibits a yellow-white hue in the core, suggesting an older stellar population, with a subtle color gradient moving outward. The outer regions display a faint and diffuse halo, lacking significant features. No obvious signs of tidal interactions or ongoing mergers are observed. The light is fairly symmetrically distributed, implying a relaxed and well-mixed stellar population. The overall smoothness of the light distribution suggests a high degree of order within the galaxy.
