The galaxy presents as an elliptical or lenticular type, displaying a smooth, relatively featureless structure. The color profile suggests a dominance of older stellar populations, with a redder hue centrally and a slight shift towards bluer tones in the outer regions. The object exhibits a high degree of central concentration, with light intensity diminishing gradually outward. No obvious spiral arm structures or dust lanes are discernible within the resolution of the image. The overall morphology appears undisturbed, showing no signs of major mergers or significant tidal interactions. There is some subtle mottling within the main body, which could indicate minor variations in stellar density or age. Based on the observed morphology and color, the object likely has a low star formation rate.
