The galaxy presents as a spiral galaxy, exhibiting a disk-like structure with a prominent bulge. The bulge appears luminous, indicating a concentration of older stars. The spiral arms appear somewhat tightly wound and the spiral arms are not very symmetric. There appears to be an indication of a possible bar feature running through the central region of the bulge. The disk shows some clumpy regions, suggestive of star-forming areas. There is a hint of blue light, particularly in areas that are not near the center of the galaxy. There do not appear to be indications of a merger. The morphology is dominated by spiral structure, with a small bulge.
