The galaxy presents as a generally smooth and rounded object, with little apparent internal structure. It appears largely elliptical in shape. The central region exhibits a high degree of concentration, with a bright core gradually fading into an extended halo. The color gradient suggests a stellar population that is predominately older and redder in the core region, transitioning to somewhat younger, bluer populations in the outer regions. There is a faint hint of possible disk-like structure, but if present it is tightly wound and viewed close to face-on. No significant signs of tidal disturbances or ongoing mergers are evident in this image.
