 This study uses Bayesian inference to demonstrate that the equation of state, EOS, of matter in the cause of maximally massive stars is consistent with quark matter, which exhibits an approximate conformal symmetry and predicts a specific form for its EOS. The likelihood of this transition is observed to correspond to EOS's exhibiting phase transition-like behavior, treated as arbitrarily rapid crossovers in the framework used. This article was offered by Emily Annala, Tyler Gorda, Janice Hervinan, and others.