We present in this paper a study of the imaging properties of the Large Binocular Telescope interfer- ometer, focusing our attention on what we believe to be the most relevant eects, namely the limited angular coverage and the partial adaptive optics (AO) correction. For this purpose we make use of the Software Package AIRY (Astronomical Image Restoration in interferometrY), designed for multiple deconvolution of interferomet- ric images and presented in our previous paper. We also consider as our testing object a model of young binary star consisting of a core binary surrounded by a massive circumbinary ring seen in scattered light, similar to that of GG Tau. The eect of angular coverage, linked to the problem of time-averaging smearing of the interferometric images, is investigated for a number of cases corresponding to dierent declinations of the observed object. We nd encouraging results showing that a good estimation of the relevant astronomical parameters of the object can be obtained even with an incomplete angular coverage. We then study the eect of partial AO-correction for both schemes of classical AO and multi-conjugate AO. We show that uniformity of the point-spread function over the eld-of-view, rather than absolute global quality, is fundamental for the quality of the restored image.