The conventional view of gravitational collapse predicts the formation of a classical event horizon (EH), followed by an inevitable singularity. However, this scenario does not fully account for the thermodynamicproperties of self-gravitating systems, particularly their negative heat capacity. In this work, we investigate how thermodynamic constraints mayinfluence the late stages of collapse and propose that a non-singular, thermodynamically stabilized intermediate state may emerge at Planck-scaletemperatures.By analyzing the temperature evolution driven by gravitational compression and energy-momentum effects, we show that the system can reachthe Planck temperature well before the classical free-fall time completes.This rapid heating phase naturally leads to a transition into a stabilizedstate supported by an Anti-de Sitter (AdS)-like interior with a negativecosmological constant. While an event horizon still forms as an observerindependent boundary, the singularity is avoided due to this internal stabilization.We further examine the holographic implications of this scenario. Theevent horizon acts not as a classical one-way membrane, but as a quantumclassical interface that stores and gradually releases information. This provides a thermodynamically motivated framework for resolving the blackhole information paradox.Rather than contradicting standard black hole physics, this model extends it by incorporating thermodynamic and quantum gravitational principles. The results suggest new avenues for theoretical and observationalexploration of non-singular gravitational collapse.