NGC 6875 is a barred spiral galaxy located approximately 90 million light-years away in the constellation Pavo. It is part of a group of galaxies known as the Pavo Group and is notable for its bright central bar structure, which is characteristic of barred spiral galaxies. The galaxy has an apparent magnitude of about 13.5, making it faint and challenging to observe with small telescopes. NGC 6875 is also home to regions of active star formation, contributing to its overall luminosity and the presence of young, hot stars within its spiral arms.