The galaxy appears to be a spiral galaxy viewed at a moderate inclination. Distinct spiral arms are visible, showing a slightly flocculent structure. The central bulge is prominent and exhibits a moderate size relative to the galactic disk. There is some suggestion of a bar feature bisecting the bulge, although it is not particularly strong. The disk exhibits a clumpy structure, potentially indicative of star-forming regions. The galaxy appears relatively isolated, showing no strong signs of major interaction or merging, although some minor disturbances cannot be ruled out. The overall color is a bluish white, suggesting ongoing star formation.
