X-ray surface brightness (left column) and spatial gradient (right column) maps of a subset of Perseus-like systems from the TNG-Cluster simulation. The gradient maps are made by applying a Gaussian gradient magnitude filter with a smoothing length σ = 2 pixels (2 kpc) to the surface brightness maps on the left column. The maps encompass a region of 200 kpc per side with a projection depth of 2 R_200c. It is noted that the color scale varies across the different clusters. Halos that exhibit closely analogous X-ray morphologies are grouped within the same row. As observed in the real Perseus, ripples, cavities or bubbles, and shock fronts are clearly visible in our simulated Perseus-like clusters at z = 0.