When we speak about entropy, it's classically defined as
$\delta S = \frac {\delta Q}{T}$
Where, I emphasize that it's the definition for only a change in entropy and not entropy itself (That's how I understood it).
And now, while speaking of the Gibbs Free Energy in Thermodynamics, I understand it as a measure of the total energy that can be extracted from a thermodynamic entity. Now, the first term in its definition accounts for the inherent energy i.e. the $U$ term (which I suppose comes from the internal thermal motion of the entity's molecules). The second term accounts for the work done on the entity i.e. the $pV$ term (energy transferred to the entity) to give it a finite volume.
Now, my confusion is with the third term, i.e. $TS$.
I suppose this definition encompasses the entropy term in its classical view because it is related to Temperature and in the Boltzmann definition, I suppose that it isn't explicitly related to Temperature.
But classically, I think, we could define only a change in entropy and not entropy itself. So what does the $S$ factor mean here? Is it Boltzmann Entropy or Classical Entropy?
If this definition is classical, then shouldn't the term actually be something like $\int T.\delta S$ with some limits thrown in because I suppose Temperature is a function of Entropy.
Where am I going wrong with these fundamentals? Also, are the two definitions of Entropy equivalent? If so, give me some helpful intuition.