Newton's second law, $F = ma$, refers to the total net force $F$ applied to an object in a given moment, and gives us it's acceleration $a$ at that moment. $m$ is the mass of the object.
The total net force $F$ is the sum of all forces acting on the object at a given moment.
Knowing only the net force $F$ (or the object's mass and acceleration, as knowing $ma$ is the same as knowing $F$), Newton's three laws do not tell us how we could obtain each individual force acting on the object.
That information is something we may obtain from analyzing the system to see which forces we expect to be acting on the object. This is called a free body diagram.
For example, for a box laying still on a table, on Planet Earth, we know (not from Newton's laws directly, but from experimental knowledge of gravity) that the Earth exerts an individual force on the box, pointing downwards, called gravity force, with a value of $F_{gravity} = m. g$, where $g = 9,8 [m/s^2]$. Since the box is still, not accelerating, we know $a = 0$ and thus $F = 0$. Therefore, there must be another individual force acting upwards on the box, with a magnitude exactly equal to $F_{gravity}$. We may call this force, normal force, and further analysis will show us that it's the table that's exerting this force on the box.
In other situations, we may be able to measure some individual forces by doing a free body diagram each other object exerting a force on our main object. If we know their acceleration, we may obtain their net $F$
Then, we use Newton's third law, that states that for every individual force $F_{a}$ exerted by A on B, there is another individual force $F_{b}$ exerted by B on A, of equal magnitude and opposite direction.
This will give us a system of equations of various net forces, and various individual forces. By solving it, we may obtain each value of interest. Of course, we will need as much information on the system as we can get.