Understanding the interactions between successive Coronal Mass Ejections (CMEs) is essential for improving space weather forecasting and mitigation strategies. When CMEs interact during their propagation through interplanetary space, their combined effects can significantly enhance geo-effectiveness, potentially triggering severe geomagnetic storms. However, the characterization and quantification of interacting CMEs, including their kinematic and magnetic field evolution and their contribution to geomagnetic disturbances, are not yet well established. By leveraging in-situ and remote observations from multiple space missions, along with numerical simulations using global magnetohydrodynamic (MHD) models, this study aims to assess CME evolution in space and time. These efforts will enhance predictive capabilities for space weather forecasting, improve our understanding of solar-terrestrial interactions, and support global space weather mitigation initiatives.