The galaxy presents as a spiral with a relatively bright, yellowish central bulge. Two prominent spiral arms emanate from the bulge region, appearing tightly wound around the central core. These arms exhibit a bluer hue compared to the bulge, suggesting active star formation within the spiral structures. The overall morphology indicates a disk galaxy seen at a slight incline, revealing some structure while not presenting an entirely edge-on view. There is an indication of a weak bar structure. The spiral arms show some patchiness, suggesting a non-uniform distribution of star-forming regions. The galaxy appears relatively isolated, with no immediately apparent major signs of ongoing merger activity, although a very minor disturbance cannot be ruled out. The bulge is small relative to the extent of the disk.
