The galaxy presents as a spiral type, with prominent arms originating from a central bulge. The bulge appears small to moderate in size relative to the overall galactic disk. The spiral arms are tightly wound around the bulge region. The color gradient across the galaxy suggests ongoing star formation, particularly within the spiral arms, with a bluer hue. There may be a weak bar feature. There is no major merging but possibly some signs of minor disturbance in the morphology.
