The galaxy presents as a spiral type, exhibiting a relatively high degree of rotational symmetry. The central bulge appears bright and concentrated, possibly indicating a significant population of older stars. Emanating from the core are spiral arms that appear tightly wound. There is a suggestion of flocculent structure within these arms. The arms display a bluish hue, suggesting ongoing star formation. The dust lanes are not clearly visible, but the overall symmetry and defined spiral structure suggests a relatively undisturbed morphology. The galaxy exhibits moderate ellipticity.
