The galaxy presents as a somewhat featureless, elliptical-like structure with a concentrated, bright central bulge. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the galaxy's light. The outer regions appear slightly fainter and more diffuse than the core, fading gradually into the background. There is no apparent dust lane or significant spiral arm structure visible, indicating a relatively smooth and evolved morphology. Minor asymmetries or subtle disturbances cannot be ruled out given the image quality, but the overall impression is that of a relaxed system.
