The large amount of data collected by current large-scale surveys will allow us to explore the properties of galaxies with unprecedented precision and help us understand their formation and evolution better than ever before. My research primarily focuses on kinematic galaxy scaling relations, which are used to measure the peculiar velocities of galaxies and thereby infer cosmological parameters. In my future research, I aim to explore how new deep imaging data can improve galaxy scaling relations, and how the full kinematic information from IFU spectroscopy can be combined with new scaling relations to obtain more accurate peculiar velocity measurements. Furthermore, given the wealth of available data, I will also study extreme and rare galaxy populations, such as red nugget relics, their formation channels, and what they can tell us about highly efficient star formation in the early Universe. In this way, my research aims to connect precision cosmology with galaxy evolution, using the same rich datasets to address both fields.