Formation energies of intrinsic defects in rhombohedral and cubic LaAlO${}_{3}$ were calculated using a first-principles projector augmented wave method based on the density functional theory. Defect energetics of single-atom vacancies, partial and full Schottky defects, and antisite cationic defects were investigated. Finite-size cell interactions in charged defects were corrected by calculating with various supercell sizes up to 480 atoms, and band-gap correction was also performed for neutral oxygen vacancy. It was found that the defect formation behaviors of both rhombohedral and cubic LaAlO${}_{3}$ are very similar to each other, that is, Schottky-type defects are preferably formed under all atmospheres and that the formation of neutral oxygen vacancies requires much more energy compared with other perovskite oxides.