NGC 5195 is a spiral galaxy located approximately 26 million light-years away in the constellation Canes Venatici. It is part of a pair of interacting galaxies, often studied for its unique structure and features. NGC 5195 is notable for its distorted shape, which is a result of gravitational interactions with its companion galaxy, M51. This galaxy has a diameter of about 30,000 light-years and is classified as a type Sc spiral galaxy. NGC 5195 is often observed in conjunction with Messier 51, also known as the Whirlpool Galaxy, which enhances its visual appeal in astronomical images. The interaction between these galaxies provides valuable insights into galactic evolution.