This appears to be a spiral galaxy, viewed at a moderate inclination. Distinct spiral arm structures are visible, exhibiting a somewhat flocculent morphology. The arms appear relatively open, with medium winding. There is evidence of substantial star formation occurring within these arms, indicated by the scattered blue regions and clumpy structure. A bar structure appears to be present across the bulge. The central bulge region has a fairly smooth, diffuse appearance, gradually transitioning into the spiral arms. The galaxy exhibits a relatively high degree of rotational symmetry. Overall, this spiral galaxy appears relatively undisturbed, and in its late stages of galactic evolution.
