The galaxy presents a distinct spiral structure, with prominent arms emanating from a central bulge. The arms appear relatively well-defined, suggesting a grand design spiral. The winding of the arms is predominantly observed to be of a medium to tight nature.

The central bulge appears moderate in size. Within the arms, there are variations in color, with regions of bluish hues intermixed with yellower tones, indicative of both ongoing star formation and older stellar populations. There are no obvious signs of a major merger event. The disk is face-on. The galaxy exhibits an inclination that allows a clear view of its spiral structure.

Based on the morphology and color distribution, the galaxy displays a moderate level of star formation activity.
