Low-resolution uGMRT images of the galaxy cluster MACS J0717+3745 showing the large-scale halo emission. The halo emission is more extended to the north and to the west than previously observed. Left: uGMRT 550−850 MHz image, which has a resolution of 10″ and a noise level of σ_{rms,  700 MHz} = 16 μJy beam⁻¹. Right: uGMRT 300−500 MHz image, which has a beam size of 10″ and a noise level of σ_{rms,  400 MHz} = 27 μJy beam⁻¹. Contour levels are drawn at [1, 2, 4, 8, …]×4.0σ_rms. In these images there is no region below −4.0σ_rms. Images are obtained using Briggs weighting with robust = 0.