Zoom on the radio relic. From left to right: highest-resolution total intensity VLA image (i.e. 3.0 GHz at 1.8″ × 1.1″; see Table 3); total averaged polarisation intensity (without correction for Ricean bias, see Di Gennaro et al. 2021c) in the 2–4 GHz band (effective frequency 3.1 GHz) at 5″ resolution; high resolution-total intensity image at 3.0 GHz with the intrinsic polarisation magnetic field vectors at 5″ resolution, corrected for Faraday rotation; optical PanSTARRS gri image with radio contours from the leftmost panel starting from 2σ_rms; Chandra 0.8–4.0 keV image with radio contours from the leftmost panel starting from 2σ_rms.