The galaxy presents as a disc-shaped structure, observed at an angle. Its overall color profile appears to be a warm yellow, suggesting a population of older stars. The galaxy's luminosity is concentrated towards the center, which fades as it extends outward. The central bulge appears smooth and featureless. The outer edges appear somewhat fuzzy and indistinct. There may be some subtle indication of spiral arm structure, but resolution is insufficient to confirm distinct arms. No dust lanes are easily identified in the images, but the galaxy itself appears relatively undisturbed. It does not appear to be undergoing any major mergers.
