Scaling relations of MaNGA galaxies color-coded by ex situ slope class, showing trends in stellar mass, star formation, rotation, Sérsic index, central velocity dispersion, metallicity, age, their gradients, bulge-to-total ratio, and 1D ex situ fraction (from Angeloudi et al. (2024)). The classes follow a sequence from low-mass star-forming rotationally supported to high-mass quenched dispersion-supported systems.