The galaxy appears to be a spiral galaxy viewed at a moderate inclination. There is a subtle, disk-like structure with a relatively smooth appearance. The central bulge is somewhat indistinct from the surrounding disk, appearing diffuse. The galaxy is elongated, suggesting a shape that deviates from perfectly round. There is a hint of disturbance or asymmetry in the spiral arms, possibly indicating a minor interaction or past merger event. The colour of the galaxy appears generally blue-white, indicating a population of younger, hotter stars and active star formation. The spiral arms are not very well defined, appearing somewhat flocculent in nature.
