One of the results of the various MCMC runs to fit a source to a lens model for MG 0751+2716. The lens model, Model 1 (shown in Table 1), from Spingola et al. (2018) was used to fit our data using the VISILENS package. The images from left to right correspond to the dirty image of the lensed source, the dirty image of the lensed source obtained by fitting the lens model, the corresponding residual map, a high-resolution model, and the source plane model.