The galaxy presents as a spiral type, exhibiting a disk structure with noticeable spiral arms emanating from a central bulge. The bulge appears substantial and is colored in yellowish-white hues, suggesting a population of older stars.

The spiral arms are well-defined, displaying a predominantly blue color, indicative of active star formation regions populated by young, massive stars. The arms appear tightly wound around the bulge, tracing a clear spiral pattern. There is some asymmetry noticeable in the arm structure.

The galaxy displays evidence of a central bar feature running through the bulge. The bar is prominent and contributes to the overall structure of the spiral arms.

The disk extends significantly beyond the bulge. It appears generally intact with no signs of a major merger event. There is no substantial dust lane visible.
