The galaxy presents as a spiral structure, exhibiting prominent and well-defined spiral arms. These arms are observed to be tightly wound around the central bulge region. The bulge appears relatively small and subtle. The arms display a bluish hue, suggesting the presence of ongoing star formation activity. The galaxy shows no signs of any major mergers, but there does appear to be another, smooth galaxy nearby which might indicate a minor interaction. Overall, the galaxy presents as a classical spiral with active star formation and a defined arm structure.
