M 106 Spiral Galaxy

Messier 106, also known as NGC 4258, is a spiral galaxy located about 22 to 25 million light-years away in the constellation Canes Venatici. It is notable for its active nucleus, prominent spiral arms, and unique water vapor maser emissions, making it an important object of study in extragalactic astronomy.



Figure 1. The M106 Spiral Galaxy

M106 is accompanied by several smaller satellite galaxies.