The galaxy presents as a somewhat elliptical, face-on system. The central bulge appears prominent and displays a concentrated, yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, there's a gradual transition to a fainter, more diffuse disk. Hints of bluer regions are visible in this outer disk, potentially indicating areas of more recent star formation. There's a subtle asymmetry to the galaxy's shape, with one side appearing slightly more extended or disturbed than the other, perhaps indicative of minor gravitational interaction. Overall the structure seems relatively smooth and lacking strong spiral arm features.
