The galaxy appears to be a spiral galaxy, though with some notable features. It exhibits a prominent disk structure, with a significant central bulge that appears moderately sized relative to the disk. The spiral arms are quite distinct, with a winding that is not overly tight nor particularly open, and is probably of the type that has two spiral arms. The light distribution suggests that this galaxy is undergoing active star formation. There is no sign of it being a pure elliptical galaxy. It exhibits some signs of possible gravitational interaction or minor disturbances. The galaxy has a bar-like structure. The estimated size is around 8 kiloparsecs.