[EDIT: Correted typos in formulae in view of #9]
From this you can only get the entropy differences, i.e.,
$$S-S_0=\frac{3}{2} n R \ln(T/T_0)+n R \ln(V/V_0)=n R \ln \left [\frac{V}{V_0} \left (\frac{T}{T_0} \right)^{3/2}\right] .$$
Now ##U=3 N k_{\text{B}} T/2## and ##n R=N k_{\text{B}}##. So you can write the above result as
$$S-S_0=N k_{\text{B}} \ln \left [\frac{V}{V_0} \left (\frac{U}{U_0} \right)^{3/2} \right].$$
Thus this is, of course, consistent with the Sackur-Tetrode formula for the absolute entropy, but the latter can only be derived by semi-classical quantum considerations, not from phenomenological classical thermodynamics.
You need in addition to the "classical fundamental Laws 0-2 of thermodynamics" also Nernst's theorem (3rd Law) as well as the indistinguishability of particles and the "natural measure" for phase-space volumes, which is determined by QT in terms of Planck's action constant, ##h=2 \pi \hbar##.
For details of a semi-classical argument for the entropy, see Sect. 1.5 in
https://itp.uni-frankfurt.de/~hees/publ/kolkata.pdf