The galaxy presents as a predominantly smooth, elliptical object. Its morphology suggests a relatively evolved system. The central region exhibits a concentrated luminosity profile, transitioning smoothly to a diffuse outer halo. There is no obvious spiral structure or prominent disk-like component visible. The color gradient implies a stellar population with older stars dominating the central regions, with a slight shift towards younger stars as you move outward. The galaxy exhibits a generally round shape, with only minor deviations from perfect circularity. There is no clear indication of any ongoing major merger events, or tidal disturbances. The overall appearance is consistent with a galaxy that has undergone significant dynamical relaxation and quenching of star formation in the central region.
