A closed universe features positive Gaussian curvature (K = +1) and can be visualized as a sphere, while an open universe has negative Gaussian curvature (K = -1) and resembles a saddle shape. The current understanding of our universe suggests it is very close to flat, with a curvature of K = 0. The geometry of the universe is influenced by its energy and matter content, with closed universes being overdense, open universes underdense, and flat universes at critical density. Einstein's General Relativity provides the framework for understanding these geometric properties. For further details, resources like Wikipedia can offer additional insights into the shape of the universe.