Despite past panchromatic observations of the innermost part of the Milky Way, the overall structure of the Galactic Centre (GC) remains enigmatic in terms of geometry. In this paper, we aim to show how 3D mapping can be used to improve our understanding of the GC. The 3D mapping technique involves creating a three-dimensional model of the GC using data from various wavelengths. This can help to identify the different components of the GC, such as stars, gas, and dust, and how they interact with each other. By studying the 3D structure of the GC, we can gain a better understanding of its evolution and how it has changed over time. Furthermore, 3D mapping can also help to identify potential sites for future astronomical observations, such as the location of black holes or other exotic objects. In this paper, we will discuss the prospects of using 3D mapping to study the GC and its potential applications in the field of astrophysics.