Pressure dependence of the thermodynamic critical field B c in elemental aluminum was studied by means of the muon-spin rotation-relaxation technique. Pressure enhances the deviation of B c (T ) from parabolic behavior, expected for a typical type-I superconductor, thus suggesting the weakening of the gap ratio α = /k B T c ( is the average value of the superconducting energy gap, T c is the transition temperature, and k B is the Boltzmann constant). With the pressure increase from 0.0 to 1.6 GPa, α decreases almost linearly from 1.73(1) to 1.67(1). Our results imply, therefore, that in elemental aluminum, the gap ratio α is smaller than the weak-coupled BCS prediction α BCS 1.764, and it is even further reduced under pressure.