Low resolution (20″) LOFAR (left) and VLA L-band (right) radio contours, superimposed on the Chandra X-ray (0.5−2 keV) image, smoothed to a FWHM of 3″. Contour levels are drawn at [1, 2, 4, 8, …] × 4σ_rms, where σ_rms at 144 MHz and 1.5 GHz are 130 μ Jy beam⁻¹ and 14 μJy beam⁻¹ respectively. The radio halo shows a strikingly similar morphology to the ICM distribution (traced by the X-ray emission), confirming the connection between the hot gas and relativistic plasma. The emission from the radio halo at 144 MHz, further extends over the whole region of detected X-ray emission. The green circle shows R₅₀₀ for the cluster.