The galaxy presents as a spiral with a prominent disk structure. The central bulge exhibits a yellowish-white hue, indicating a population of older stars. Faint spiral arms extend from the core, showcasing a bluish tint, suggesting active star formation regions. Patches of red are observed within the arms, implying the presence of dust lanes or regions of intense H-alpha emission possibly due to recent starburst activity. The arms appear somewhat tightly wound. The galaxy is not perfectly face-on, exhibiting a slight inclination with an ellipticity of around 0.8, and a median radius of 7.3 kpc.
