The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a bright, compact core exhibiting a pale yellow-white hue, indicative of an older stellar population. Surrounding the core is a more diffuse halo exhibiting a slight gradient, transitioning to a bluish color in the outer regions. This may suggest ongoing, albeit limited, star formation or perhaps a population of younger stars compared to the core. There is no evidence of distinct spiral arms or a prominent disk structure. No apparent tidal features or signs of major interactions with neighboring galaxies are observed, though minor disturbances cannot be ruled out at this resolution. Overall, the galaxy appears to be a relatively undisturbed, massive system.
