The galaxy presents as a slightly elliptical, face-on system. Its core exhibits a brighter, concentrated luminosity, suggesting a possible central bulge. The overall light distribution appears relatively smooth. The edges fade gradually without sharp boundaries. The galaxy's color profile indicates a bluer hue in the outer regions and a slight shift toward redder tones toward the center. There might be subtle irregularities in the disk, but overall, the galaxy does not present a strong spiral or barred structure. It shows a fairly regular structure with only minor distortions, but the possibility of a small interaction cannot be ruled out.
