The galaxy presents as a spiral type. There is a prominent, moderately sized central bulge with a yellow-white hue. The disk appears inclined relative to our line of sight, but it is not fully edge-on. Spiral arms are visible, displaying a two-armed morphology. They emanate from the central bulge. The spiral arms demonstrate a medium winding, showing a clear but not tightly wound structure. The arms exhibit a bluer color, indicating the presence of younger stellar populations. No strong bar structure is apparent in this image, although there may be a very weak bar component. There are some indications of minor disturbances or interactions, but no major merger event seems to be occurring.
