This galaxy exhibits a spiral structure, with prominent, well-defined arms. These arms are slightly offset or distorted. The galaxy has a substantial central bulge. It is moderately bright. The arms display clumpy regions, possibly indicating zones of active star formation. The galaxy appears to be undergoing some form of interaction or disturbance based on the structure of the spiral arms. There is evidence of a disk. There is a faint object close to the galaxy, with a strong possibility that it is merging with the larger galaxy.
