The galaxy appears to be an elliptical galaxy with a smooth, concentrated light profile. Its core is a bright, yellowish-white, indicating an older stellar population. There is a slight elongation along one axis but overall has a relatively round shape. The galaxy shows no signs of spiral arms or active star formation regions. The color gradient suggests a gradual decrease in stellar age from the core outwards. There is no evidence of significant tidal disturbances or recent merger activity visible in this image.
