The galaxy appears as a singular, concentrated body of light with an elliptical morphology. It exhibits a smooth, rounded profile, with no discernible spiral arms or distinct features. The color gradient suggests a relatively uniform stellar population, with a concentration of older, redder stars towards the core and slightly bluer tones in the outer regions. There is no clear evidence of ongoing mergers or major disturbances in the galaxy's structure. The galaxy presents a high degree of central concentration, with luminosity gradually decreasing with radial distance from the center. Overall, it is well structured with an even light profile and a large rounded shape. 
