This is a colour photo from the VLT that shows NGC 4650A, a member of the so-called Centaurus chain of galaxies in the southern constellation of that name. NGC 4650A is a complex system that is located at a distance of about 50 Megaparsec (165 million light-years). As it is clear from this high-resolution picture, there are two main components, a lenticular-shaped galaxy (of type S0), surrounded by a knotty extended ring-like distribution of stars, dust and gas, nearly perpendicular to each other. The stars in the central, structureless region and the material (stars, gas, and dust) in the outer disk rotate in two different planes that are nearly perpendicular to each other. The observed motions indicate the presence of a significant halo of dark matter within the system, although it is still unclear to which of the two components this matter belongs. Because the velocities of stars and gas can be measured in two independent planes, NGC 4650A serves as a prototype for detailed studies of the shape of dark matter halos. The origin of this strange spatial configuration is not known with certainty. It is likely, however, that an encounter between two galaxies may have played a significant role