The galaxy appears to be an elliptical galaxy, characterized by a smooth, symmetrical light distribution with a relatively round shape. It displays a color gradient, with a central yellowish-orange hue transitioning to a bluish-white periphery. This suggests a concentrated population of older, redder stars in the core, while the outer regions show evidence of a younger, bluer stellar population, indicating ongoing star formation. There are no discernible spiral arms or a prominent disk structure. No major disturbances or signs of merging are obviously visible. 
