Confusion matrices showing the results before and after the TL process of predictions of stellar streams in galaxies at different inclinations. The first and second rows correspond to the SAD-CNN results before and after TL, respectively. Each column represents a different inclination angle from Group III, with the last column presenting the results for the combined sample. The rows inside the matrix represent the true labels of the galaxies, meanwhile, the columns represent the predicted labels of the model. The matrix to the right in both cases presents the complete sample with all inclinations.