LOS velocity dispersion profiles from the stellar kinematics of the BCG, obtained by extracting spectra in elliptical radial regions from the MUSE data cubes, independently in the NE (red circles) and SW (blue squares) portion of the BCG, as shown in the inset. The latter is a median stack of the MUSE data in the inner 30 arcsec around the BCG, with projected faint cluster members masked out in the spectral extraction. We note that the innermost radial bin (blue) in the SW side of the BCG is excluded since it contains the gap between the two MUSE pointings. Vertical dashed lines indicate 1,2,3 effective radii (R_e = 17 kpc).