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We established a separation scheme to distinguish galaxies from stars with the aid of AKARI/FIScolor-color (CC) diagrams. In all the combinations of CC diagrams we can distinguish two separateclouds. It was shown that in all cases one of them contains more than 95% of galaxies and theother one, in most cases, consists in more than 80% of stars (Pollo et al., 2010). Currently weare looking into more detailed classications. We are especially interested in separating dierentmorphological types of galaxies, mainly within spiral galaxies. Moreover, we study the propertiesof infrared galaxies. Key words: infrared: galaxies, stars; telescope; conferences: proceedings1. OUR SAMPLEIt is crucial for all-sky surveys, detecting tremendousamount of sources, to nd a way to distinguish betweendierent kinds of objects based on minimal amount ofadditional information. The best option would be touse only data which is brought by the survey itself.The AKARI/FIS catalogue contains more than400,000 sources. For the reason mentioned above,we are looking for various classication schemes be-tween dierent types of objects within the catalogue,using photometric information only. For our pur-pose, we selected sources in regions of low Galacticemission at 100

CLASSIFICATION SCHEMES AND PROPERTIES OF INFRARED GALAXIES