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Key questions formulated decades ago are nevertheless not satisfactorily answered. What are the main drivers determining the morphology of galaxies, which are responsible for establishing the Hubble sequence? When did this happen? What is the role of acquired angular momentum in shaping galaxies? Is the downsizing and early quenching of star formation in massive systems due to AGN feedback, as commonly assumed, or to reduced gas infall from cosmic flows, or to both? .