Redshift evolution of cluster entropy (top) and temperature (bottom) profiles. The left panels stack the full TNG-Cluster sample based on four halo mass bins (log₁₀(M/M_500c) ranges in legends), while the right panels separate the full sample into its SCC, WCC, and NCC sub-populations. In both cases, we bin in mass or classify CC state at each of z = 0, z = 0.2, z = 0.5, and z = 1 separately. The entropy profiles shift downward with increasing redshift and decreasing halo mass while maintaining a similar shape. The temperature profiles strongly depend on mass and weakly on the redshift. At all redshifts, the entropy profiles for CCs and NCCs are well separated in the core, while the temperature profiles are not and show a large scatter.