The galaxy exhibits a disk-like morphology with evidence of spiral arm structure. The arms appear somewhat flocculent, lacking well-defined continuous structures. The central bulge is not particularly pronounced. There is a clear blue color, indicative of on-going star formation within the arms. The galaxy does not appear perfectly face-on; it presents a slight inclination relative to our line of sight. There is no bar-like structure visible in the central region. There is a slight distortion visible in the structure of the disk, but no obvious signs of a major merger. There are some faint asymmetric extensions which could be the result of tidal interactions with smaller companions or some disturbance.
