The unit $\mathrm{mol}$ is dimensionless. It refers to a countable, integral number of a thing. It's like counting in 100s, except $1 \mathrm{mol}$ is larger. $1 \mathrm{mol}$ is an integer, equal to about
$$1 \mathrm{mol} \approx 6.022 \times 10^{23} \, .$$
The number on the right is called the Avogadro Constant.
The $\mathrm{mol}$ is conventionally used in chemistry to count the number of molecules, or the number of atoms. That's really it. It's more convenient to count in numbers of moles because $1 \mathrm{mol}$ of common compounds and atoms are an easily imaginable mass-- i.e., $1 \mathrm{mol}$ of hydrogen atoms about $1 \mathrm{gram}$.
If you want to be pedantic, the number of moles of something may not be well-defined because the substance may be in a superposition of different particle-number states. But this is always ignorable in practical uses of the unit $\mathrm{mol}$.
If you want to be pedantic in a different way, the word 'scalar' is used in physics to refer to members of $\mathbb R$ or $\mathbb C$. In more advanced physics, the word 'scalar' is used as a description of a mathematical entity's transformation properties. For example, a 'scalar field' is a field which doesn't change value at any point as a result of spatial transformations which scale the coordinates. The points move around but internally the scalar value doesn't change, it just shifts around. On the other hand, a scalar density is a quantity which is defined to stretch/squeeze with the coordinate system, in such a way that if you integrate over a given volume, that integral will be preserved even under a coordinate transformation.
The reason that scalars and scalar densities have so much salience to us (i.e., they are intuitive) is because locally (which is what our classical brain is attuned to-- variations in spacetime are not large enough for us to really observe in a visceral and immediate sense), all spacetimes are Minkowskian (flat spacetime). And all of the isometric transformations you can do on a Minkowskian spacetime (Poincare transformations) happen to have no effect on scalars or scalar densities. I.e., if you and I are using different coordinates on the same shared space, then regardless of our coordinate choices, we agree on the value of scalars and scalar densities. (I have ignored Lorentz boosts, since we don't have classical intuition for those either).