Stellar kinematic maps of the galaxy FCC 47 and its NSC overplotted with the isophotes of the IFU white-light images. The panels show from top to bottom the mean velocity, velocity dispersion, and h₃ and h₄ Gauss-Hermite higher-order velocity moments. From left to right, we show the central 3 × 3 arcsec extracted from the SINFONI observations, and the MUSE kinematics within the central 14″ × 14″ and across the 60″ × 60″ MUSE FOVs. SINFONI and MUSE kinematics are shown with different mean velocity and velocity dispersion scales due to the different spatial resolution. The host galaxy rotates significantly slower than the NSC (r_eff = 0.7″) in the centre of FCC 47. North is up and east to the left.