The galaxy appears as a centrally concentrated, luminous object. It exhibits a relatively smooth morphology with an overall elliptical shape. The light distribution suggests a more rounded structure than a highly elongated one. There is subtle evidence of a possible disk-like component, although the dominant characteristic is that of a smooth spheroidal system. No signs of strong tidal disturbances or recent merger events are apparent. Color gradients across the galaxy are subtle but present, with a slightly bluer hue in the central regions gradually transitioning to redder colors towards the outer parts. This may indicate ongoing star formation in the central regions while older stellar populations dominate the outskirts. The galaxy's estimated physical size is consistent with that of a typical galaxy.
