This galaxy presents as a spiral galaxy with a moderate to high degree of observed disk structure. A central bulge region is noticeable, displaying a yellow/orange hue, indicative of an older stellar population. Faint spiral arms are present and tightly wound around the central bulge. The spiral arms have a distinct blue tint suggesting the presence of younger, hotter stars and ongoing star formation activity. There is no visible sign of any major galaxy merger or disruption.
