The galaxy presents as a spiral type, with a relatively bright, moderately sized central bulge. Two prominent spiral arms emanate from the central region, winding outward in a grand design. These arms appear somewhat flocculent and are not tightly wound, displaying a medium pitch angle. There is a hint of a bar-like structure. The disk shows color variation, with bluer regions associated with the spiral arms suggestive of on-going star formation. The bulge exhibits a more yellow/red hue, indicating an older stellar population. The overall appearance suggests a well-formed galaxy with active star formation in its spiral arms. There are no obvious signs of major mergers or significant tidal disturbances, although a minor asymmetry or disturbance within one of the arms could be present.
