The galaxy presents a primarily face-on orientation, exhibiting a disk-like structure. Spiral arm features are visible, though somewhat flocculent and not sharply defined. There appears to be a central bulge, though it is not overly dominant within the galaxy's overall structure. The color profile suggests ongoing star formation, with bluer hues prominent in the spiral arms. There are no indications of a major ongoing merger event, though there appears to be some morphological disturbance within the spiral arms, suggestive of minor interactions or internal dynamics. The galaxy does not appear to have a strong central bar feature. The overall impression is of a spiral galaxy with moderate star formation and some morphological irregularities.
