It's a complicated question.
The Moon orbits the Earth. The Earth in it's turn orbits the Sun and the Sun orbits the Galaxy center. Orbits are only approximately circular. They are actually ellipses. Moon and Earth are both rather circular in their orbits, but not actually circles.
In a circle, the outer edge of the circle always has a constant distance from the center or focus. In an elipse, the outside always has a distance from the two focii that is a constant, but it is the sum of the two distances that is the constant.
Then, where you are on the Earth matters. Plus, the Earth is tilted with respect to the Moon and the Sun. Your specific latitude also matters, as you see the moon from a position that moves relative to the actual position of the Moon during the day/night. But the Moon has also moved during that time, as has the Earth. Then again, just how your part of the Earth is tilted as you look at the Moon varies with the seasons as well.
This just gives some of the considerations. To really answer the question would take 3D Trigonometry and some Solid Geometry. Those two subjects come together in Analytic Geometry, which is covered in second year Calculus and which is beyond anything that belongs on this website.
I would suggest you write off to a planetarium. Illustrating things like this is part of why they exist. New York has a good one, Neil DeGrasse Tyson runs that one and has a good reputation.