The galaxy presents a smooth, elliptical morphology, appearing largely featureless within the limits of this image resolution. Its overall shape approximates a spheroid, with minimal discernible disk structure. The central region exhibits a pronounced luminosity, suggesting a high stellar density and potentially an active galactic nucleus. The color profile shifts gradually from a golden hue at the core to a redder shade in the outer regions, indicative of an aging stellar population. No significant tidal features or signs of recent major merger activity are apparent, suggesting a relatively undisturbed evolutionary history. The overall color and morphology suggest a massive system, likely at a significant distance.
