The galaxy presents as a relatively smooth, centralized luminous structure, likely an elliptical or lenticular galaxy viewed at a significant distance. The core exhibits a yellowish-white hue, suggesting a population of older stars. There is little evidence of prominent spiral arms or active star formation regions from the image. The outer regions appear fainter, fading gradually into the background with a round morphology. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, maintaining a settled and relatively undisturbed form.
