The galaxy presents as an elliptical structure with a smooth, largely featureless morphology. The central region exhibits a bright, concentrated core, indicative of a significant stellar population possibly due to the presence of a supermassive black hole. Proceeding outward, the galaxy gradually fades into a more diffuse halo. The color profile shifts from a yellowish-white core to a bluish halo. This suggests that the outer regions may contain a younger stellar population or the effects of dust scattering blue light. Overall, the galaxy exhibits a shape that is neither perfectly round nor highly elongated, but rather an intermediate elliptical form, with no signs of major disturbances or mergers.
