Galaxies are large clusters of stars, solar systems, gas, and dust held together by gravity. Using the Hubble Space Telescope, astronomers estimate that there may be 100 billion galaxies and probably more. Galaxies are classified based on their morphology and are divided into three major categories: elliptical, spiral, and irregular galaxies. As mentioned in previous chapters, we live in the Milky Way galaxy, a spiral-type galaxy. However, a lot of galaxies also appear in unusual forms, usually a combination of the main morphologies.