The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. Its overall shape appears round to slightly elliptical. The central region exhibits a brighter, more intense yellow-white hue, indicating a high concentration of older stellar populations. Moving outwards from the core, the galaxy shows a gradual decrease in luminosity and a shift toward a more diffuse, reddish-tinged color. This color gradient suggests a possible decline in star formation rate with increasing distance from the galactic center. There is no apparent spiral structure or prominent dust lanes discernible in this image. Overall, the galaxy's appearance is indicative of a mature system with characteristics leaning towards an elliptical or lenticular type. There is no major merger activity visually apparent, though subtle disturbances cannot be ruled out.
