NGC 4330 is a spiral galaxy located in the constellation Virgo. It is approximately 55 million light-years away from Earth and is part of the Virgo Cluster, a group of galaxies that are gravitationally bound together. This galaxy is notable for its distorted shape, which is thought to be the result of interactions with other galaxies in the cluster. Observations of NGC 4330 have provided insights into the effects of environmental factors on galaxy evolution, making it an important subject of study in astrophysics.