The observed galaxy exhibits a disk-like structure with prominent spiral arms. The arms appear somewhat flocculent, displaying distinct regions of star formation. The galaxy's color suggests a population of both young, blue stars and older, redder stars distributed throughout. A central bulge is not strongly apparent; instead, the galaxy appears more diffuse towards its center. Evident are indications of potential gravitational interaction or recent merger activity, exhibiting possible tidal features or disturbances in the spiral arm structure. There are possible signs of a weak bar structure visible within the central region of the galaxy.
