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Till now, 157 globular star clusters (GSCs) were revealed in the Galaxy, and there is a large bank of observation data for them, which have been collected for a long time (see, e.g., catalog [1] and references therein). A lot of works are devoted to theoretical aspects of the origin and evolution of GSCs. Nevertheless, the problem of GSC classification still remains open, although some of well-known authors tried to solve it. In order to understand the current state of the problem of GSC classification, it is necessary at first to present here, at least briefly, the main results obtained in this area. First of all, the proposition made by Shapley and Sawyer [2] should be mentioned. The cited authors were first who proposed to classify GSCs according to the degree of apparent star concentration toward the cluster center. They introduced 12 classes of concentration toward the center and denoted them using Roman numerals. For this purpose, they firstly created an almost uniform series of photos for 103 GSCs. Class I included clus-

Can Globular Clusters in the Galaxy Be Classified by the Velocity Anisotropy Parameter?