Black holes represent the most extreme gravitational systems known and are commonlyassociated with horizons, strong spacetime curvature, and the breakdown of classical descriptionsat singularities. In conventional treatments, these features are often regarded as indicators ofincomplete physics or as requiring fundamentally quantum explanations. Within the Theoryof Imbalance of Energy (TIE), black holes are reexamined as natural saturation regimes ofinteraction imbalance accumulation.Building on the interpretation of gravity as large-scale accumulation of slowly redistributinginteraction imbalance, this paper argues that black holes form when imbalance accumulationapproaches the limit of redistribution capacity. In this regime, redistribution becomes stronglysuppressed, external influence decouples from internal dynamics, and effective geometric descriptions reach their limits of applicability. Horizons arise as redistribution boundaries ratherthan as fundamental geometric surfaces, and information is stored within internal imbalanceconfigurations rather than destroyed.The analysis remains entirely classical, deterministic, and causal. No modification of established gravitational predictions is proposed. Instead, black hole features such as horizons,time dilation, apparent information loss, and evaporation are interpreted as consequences ofsaturation and delayed redistribution within a unified interaction framework. The results establish conceptual continuity between ordinary gravitational systems and extreme regimes withoutinvoking physical singularities as fundamental entities.