In general relativity (GR), the gravitational constant G serves as a conversion factor between conventional units and geometric units, maintaining its role from Newtonian mechanics but without implying a force. G appears in Einstein's field equations, linking the energy-momentum tensor with the curvature of spacetime, but its significance is more about unit consistency than a physical property of spacetime itself. While some argue that G could represent curvature effects, it fundamentally functions as a proportionality constant necessary for the equations to align with observational data. GR does not treat gravity as a force, complicating the interpretation of G's meaning compared to Newtonian gravity. Ultimately, G retains its value and meaning across both theories, primarily as a unit conversion tool rather than a direct representation of gravitational interactions in GR.