Spatial distribution of cluster galaxies is shown with red circles for quiescent galaxies from our spectroscopic sample and blue stars for the star-forming ones, while green points mark spectroscopic cluster members from the literature. Light-grey contours indicate the galaxy number density of the spectroscopic members, while magenta contours show the XMM X-ray emission within 2r₂₀₀. The top-right X-ray emission is at the edge of XMM coverage and needs further analysis. No in-falling groups were detected (except the core), as the X-ray peaks do not coincide with the galaxy overdensities.