The galaxy presents as a spiral galaxy with a clearly defined, albeit somewhat flocculent, spiral arm structure. A central bulge is apparent, appearing to be a moderate size relative to the disk. There is a suggestion of a weak bar feature bisecting the central bulge. The galaxy exhibits a blue hue, which is probably indicative of recent star formation within the spiral arms, and it also seems that it could be undergoing a minor merger or tidal interaction with another galaxy. There is a noticeable asymmetry in the outer regions of the galaxy, with a faint extension or distortion visible on one side, implying possible gravitational disturbance. The galaxy is not seen edge-on.
