The galaxy appears as a centrally concentrated, nearly circular object with a smooth morphology. The light distribution suggests a relatively uniform stellar population. The object exhibits a color gradient, appearing bluer toward the outer regions and redder towards the center, possibly indicating younger star formation in the outskirts and an older, more evolved stellar population in the core. There is no evidence of spiral arm structure, bar features, or significant tidal disturbances. The overall appearance suggests a classification as an elliptical galaxy or a lenticular galaxy viewed close to face-on. The light appears to fade smoothly from the bright center, hinting a gradual decrease in stellar density with increasing radial distance.
