This galaxy exhibits a distinct spiral structure with well-defined arms. The arms are somewhat patchy in appearance, suggesting ongoing star formation activity. The central bulge is not prominent; instead, it appears small or possibly non-existent. The galaxy displays a blue hue, especially prominent in the spiral arms, consistent with a population of young, hot stars. There is evidence of minor distortions or tidal features, potentially indicating recent or ongoing interactions with another galaxy. While the majority of the galaxy appears relatively undisturbed, there are hints of disturbance within the overall structure. No obvious bar structure is apparent. The galaxy appears to be relatively face-on from our point of view.
