Vertical slices through the galactic disks of the CRMHD (left) and the MHD (right) simulations at t = 1 Gyr. Both panels show the hydrogen number density on their left and the gas temperature on the right half, respectively. Accounting for CR feedback results in a visually distinct inner CGM around the galaxy. The simulation which includes CRMHD physics has a denser and colder CGM and appears to be more turbulent in comparison to the MHD simulation.