The galaxy displays a disk morphology with evidence of spiral arm structure. The spiral arms appear somewhat flocculent, lacking grand design coherence. There is a central bulge region, appearing moderately sized relative to the overall galactic disk. The galaxy presents with a noticeable amount of disk inclination but is clearly not an edge-on system. There is some degree of irregularity or disturbance visible within the galactic structure suggesting possible past or ongoing minor merger activity.
