The galaxy presents as a somewhat face-on spiral, exhibiting prominent spiral arm structures that emanate from a central bulge. The arms appear grand design but are flocculent, showcasing significant star formation regions, indicated by bluish hues and knotty features throughout their extent. Dust lanes are observable along the inner edges of the spiral arms, contributing to a complex interplay of light and obscuration within the galactic disk. The central bulge appears moderately bright and concentrated, its light profile suggesting a relatively high stellar density in this region. Overall, the galaxy is disk-dominated with a bulge, indicative of a system where ongoing star formation and spiral arm activity are significant contributors to its overall morphology.
