The galaxy appears as a roughly elliptical, centrally concentrated object. Its light profile suggests a smooth and diffuse structure. Color gradients are subtle, with a slightly more yellow-white core transitioning to a bluish periphery. There is no clear evidence of spiral arms or a prominent disk, which are generally bluer and more distinctly defined compared to the core. There are no obvious signs of recent or ongoing major mergers, but the galaxy could potentially be experiencing some minor interactions, though further data would be necessary to confirm. The overall appearance suggests a relatively evolved system, potentially an elliptical galaxy undergoing star formation.
