NGC 6876 is a barred spiral galaxy located approximately 90 million light-years away in the constellation Pavo. It is part of the Pavo group of galaxies and is notable for its bright core and well-defined spiral arms, which are rich in star formation. This galaxy has an apparent magnitude of about 12.5, making it a faint object that requires a telescope to observe. NGC 6876 is also classified as a Seyfert galaxy, indicating that it has an active nucleus with strong emission lines, suggesting the presence of a supermassive black hole at its center.