The galaxy appears to be a spiral galaxy, exhibiting a prominent disk structure with clearly defined spiral arms. The arms display a tightly wound morphology. The central bulge appears moderate in size and exhibits a yellowish-white hue, suggesting an older stellar population. The disk shows a bluer color, indicative of ongoing star formation and a younger stellar population. The galaxy does not appear to be significantly disturbed or undergoing a major merger. The galaxy presents a relatively high degree of axisymmetry, with a minor axis close to the major axis.
