Same format as Figure 6, now shown for TN J0121+1320. The source exhibits a compact radio morphology, marked by the green star. The radial profiles reveal sharp enhancements in both the mass outflow rate and kinetic power at ∼15 kpc, closely corresponding to the radio position, though possibly slightly offset. Due to the unresolved radio morphology and lack of an extended jet axis, the jet-gas interaction is unclear.