The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population and minimal ongoing star formation. The light smoothly decreases radially outward from the core, displaying a diffuse, ellipsoidal halo. The galaxy appears relatively smooth and undisturbed, lacking prominent spiral arms, dust lanes, or other features typically associated with recent merger events. The overall color gradient suggests a gradual decline in stellar age and metallicity from the core to the outer regions. There is a slight flattening of the galaxy, suggesting that it isn't perfectly spherical. The galaxy's color indices suggest that the galaxy contains stars of varying ages.
