Nearelliptical

Near-elliptical galaxies are a type of galaxy that are similar to elliptical galaxies but have a slightly more flattened shape. They are characterized by their smooth, featureless appearance and lack of distinct spiral arms. Near-elliptical galaxies are often found in the centers of galaxy clusters and are thought to be the result of mergers between spiral galaxies. They are typically larger than elliptical galaxies and have a higher concentration of stars in their centers. Near-elliptical galaxies are classified as S0 galaxies in the Hubble sequence. They are an important object of study in astronomy, as they provide insights into the evolution of galaxies and the processes that shape their structure.