1 INTRODUCTION  
2 DATA  
2.1 The SAMI Survey  
2.2 The HSC SSP Survey  
2.3 Sample Selection  
2.4 HSC Surface Brightness Limits  
3 METHOD  
3.1 MGE Galaxy Profile Modelling  
3.2 Model Subtraction and Visual Inspection  
4 RESULTS  
5 DISCUSSION  
5.1 Effectiveness of Visual Classification  
5.2 Interpretation of Hα Equivalent Widths  
5.3 The Role of Galaxy Mergers in Kinematic Evolution and the Formation of Slow Rotators  
5.4 Comparison of SAMI, MATLAS and Magneticum  
5.5 Radial Infall Galaxy Mergers  
6 CONCLUSIONS