Full-resolution (9″ × 6″) LOFAR image overlaid on an exposure-corrected, background-subtracted Chandra image in the 0.5–2.0 keV energy band with a total integration time of 22.9 ks. The LOFAR contours (white) show the (1, 2, 4, …)×5 × σ_LOFAR levels and the dashed white contours show the −3σ_LOFAR, where σ_LOFAR = 150 μJy beam⁻¹. The cyan contours are the weak lensing measurements showing the dark matter distribution. The star, square, and triangle show the peak of the dark matter distribution, X-ray peak, and radio peak, respectively. The solid black and dashed black line show the tentative location of the shock and cold front suggested by Botteon et al. (2018a).