The galaxy presents as a relatively bright, face-on spiral structure. There is a moderate bulge with a notable disk. Spiral arms are visible, exhibiting a somewhat flocculent nature. Subtle features are present in the arms, suggesting active star formation regions, indicated by slightly bluer hues. The disk is quite prominent and dominates the galaxy's overall visual footprint. The galaxy does not appear to be undergoing a major merger, though subtle irregularities hint at a possible minor disturbance. A bar structure might be present. The galaxy's ellipticity is relatively low.
