The galaxy presents as a spiral structure, viewed face-on. The central bulge appears yellowish, indicative of an older stellar population. Faint spiral arms are visible, extending outward from the bulge, these arms have a relatively fragmented appearance. The arms display a bluish tint suggesting the presence of younger, hotter stars and ongoing star formation. The winding of the spiral arms appears relatively tight. There is no clear bar structure visible. The overall color of the galaxy suggests it is a mature spiral galaxy with both ongoing star formation and a significant population of older stars. There is no obvious indication of major mergers or tidal disturbances, although some subtle irregularities in the spiral arm structure may indicate minor interactions. The absence of a strong central dust lane suggests a relatively low dust content overall.
