A new preprint from the MELIORA hydrodynamical suite argues that the ultraviolet diversity of JWST-discovered Little Red Dots encodes the ages of embedded direct-collapse black holes. The simulation tracks the first ~30 Myr after DCBH formation, showing a rapid shift from BH-dominated, metal-poor systems with high Eddington ratios to stellar-dominated hosts with rising metallicity and lower BH-to-stellar mass ratios. This evolutionary sequence is presented as a testable prediction for emission-line ratios and continuum slopes. Because the study is simulation-based rather than observational, it carries the usual caveats of sub-grid prescriptions for Pop III star formation and accretion physics; no direct count of objects is provided. Earlier JWST analyses (e.g., Labbe et al. 2023) noted the compact, red continua but stopped short of mapping them onto DCBH formation channels. Inayoshi et al. (2020) had outlined the theoretical conditions for direct collapse yet lacked observable diagnostics. The MELIORA results therefore bridge these threads by predicting that UV-brighter LRDs should host older seeds—an insight most reporting has treated as speculative rather than falsifiable. The short ~30 Myr LRD window also tightens the required duty cycle for DCBH emergence at z>8.5, a constraint rarely quantified in observational summaries.