Projected kinematics of NGC 4993, inferred from MUSE data (top row) and predicted by JAM (bottom row). The left column shows the mean stellar velocity, V, along the LoS, while the right column shows the rms velocity, V_rms, along the LoS. The solid black lines represent the observed isophotes (top row) and the MGE fit (bottom row). The x′ axis is aligned with the galaxy photometric major axis.