This paper synthesizes the modern understanding of the Universe’s large-scale structure and its origin. We describe the hierarchical organization of matter, ranging from planetary systems to the immense, foam-like Cosmic Web composed of filaments, nodes, and voids. On scales larger than approximately 300 Mpc, this structure transitions to statistical homogeneity, a regime known as the “End of Greatness” [citation:3]. The theoretical foundation for this structure is the Lambda Cold Dark Matter (ΛCDM) model, in which the gravitational amplification of primordial quantum fluctuations—stretched to macroscopic scales by cosmic inflation—seeds all subsequent structure formation. We review the key observational pillars supporting this framework: the near-perfect blackbody spectrum and minute anisotropies of the Cosmic Microwave Background (CMB) [citation:2], large-scale galaxy surveys that map the Cosmic Web [citation:3], and the gravitational evidence for non-baryonic dark matter. Finally, we discuss persistent challenges to the standard cosmological paradigm, including the Hubble tension and the unknown fundamental nature of dark matter. These open questions underscore cosmology’s status as a precision science, poised for transformative discoveries with the advent of next-generation observatories.