The galaxy appears to be a spiral galaxy, oriented face-on. Two prominent spiral arms emanate from the central bulge region. These arms are moderately wound, exhibiting a medium pitch angle. The galaxy displays a strong blue color gradient in the spiral arms, suggesting ongoing star formation activity. The central bulge appears yellowish, indicating a population of older stars. No bar structure is readily apparent. The galaxy shows no strong evidence of recent or ongoing major merger activity, though some minor disturbances may be present in the outer regions of the disk. The overall morphology suggests a relatively normal spiral galaxy with moderate star formation. The color profile suggests the galaxy has been forming stars for a while, but still has plenty of gas.