Morpho-kinematic evolution diagram along the Fall relation. The average M_★ and j_★ for each morpho-kinematic class, and their 1σ standard deviations, are represented following the colour and marker scheme introduced in Fig. 3. The stellar sAMSD maps for the representatives of the five j_★ types are arranged on the j_★-M_★ plane in the location corresponding to their stellar disc mass and total stellar sAM. Each galaxy is labelled according to its morpho-kinematics. Starting from the lower-left corner and moving up along the best-fit line for our sample, we have UGC8490, UGC10359, UGC10470, UGC6537, and UGC9969. The axes and the parameters in the upper-left corner are the same as in Fig. 3.