The galaxy presents a clear disk morphology, observed at a moderate inclination. Spiral arm structures are readily apparent, exhibiting a somewhat flocculent nature. These arms appear to be relatively open and extend outwards from the central region of the galaxy. A distinct, bright central bulge is evident; however it does not dominate the galactic structure. There may be a slight distortion, indicating possible gravitational interaction but no significant major merger. The galaxy appears to have a substantial amount of gas and dust present. It is of moderate size.
