The galaxy appears as a moderately bright, elliptical-shaped object. Its light profile suggests a smooth, continuous distribution without obvious spiral arm structures or a prominent central bulge. The galaxy exhibits a color gradient, appearing somewhat bluer toward its outer regions and redder in its central area, which is possibly indicative of an older stellar population concentrated towards the core. There is a slight asymmetry that may point to some sort of disturbance, but it is difficult to determine a potential cause. I do not observe any signs of active galactic nuclei or distinct morphological features typically associated with ongoing mergers, though minor tidal disturbances cannot be fully excluded.
