The galaxy presents as a spiral type, though the inclination is not edge-on. Distinct spiral arms are observable emanating from the central bulge. The arms appear somewhat flocculent and not as tightly wound. The central bulge is a moderate size, appearing neither extremely dominant nor negligible in proportion to the disk. There is no strong evidence of a central bar structure. The disk exhibits a generally blue hue, contrasting with the yellower, more concentrated light from the bulge, suggesting ongoing star formation within the disk. There is no immediately obvious signs of major disturbances or advanced merging activity, though some minor irregularities in the arm structure might suggest past interactions or minor tidal distortions. The overall light distribution is relatively smooth, but not completely uniform. The color distribution may suggest the central bulge consists of older stars.
