The galaxy presents a flattened, elliptical morphology. The central region exhibits a concentrated, bright core, appearing a yellow-white hue. This suggests an older stellar population dominating the core. The galaxy lacks discernible spiral arm structure or prominent dust lanes. There are no clear signs of active galactic nuclei activity visible in this image. The surrounding halo appears smoother and more diffuse, with a slight fading to a faint blue. The overall structure indicates a relatively evolved system with a substantial spheroidal component. There are no obvious signs of a major merger in progress.
