The most widely accepted geometries of the universe include Euclidean geometry, which describes flat space, and non-Euclidean geometries like elliptical (Riemann) geometry, which accounts for curved space. Current models suggest the universe is expanding with spatial slices of constant comoving time that are predominantly flat. However, measurements indicate a slight possibility that the universe could also exhibit a 3-sphere or open hyperbolic geometry, both with a very large radius of curvature. This means that while the universe appears flat, there is still room for alternative geometrical interpretations. Understanding these geometries is crucial for comprehending the overall structure and evolution of the universe.