The galaxy presents as a spiral galaxy with a defined disk structure. The spiral arms appear to be moderately wound, exhibiting a discernible, but not tightly wrapped, pattern around the central bulge. Two spiral arms seem to be prominent in the image. The bulge appears relatively small in proportion to the disk size. The galaxy does not appear to be undergoing any major merging activity, although some minor disturbances may be present in the disk, possibly indicating ongoing interactions. The axial ratio of the galaxy suggests it is viewed at a slight inclination, but not edge-on. The overall color of the galaxy indicates a bluer hue, suggestive of active star formation, particularly within the spiral arms.
