The galaxy presents a smooth, elliptical morphology. The core region exhibits a concentrated, bright, yellowish-white glow, indicative of a high stellar density and potentially an older stellar population. Moving outward from the core, the color gradually shifts towards a reddish hue, suggesting the presence of relatively aged stars. There are no discernible spiral arms or dust lanes within the resolution of this image. The galaxy appears generally undisturbed, showing no significant signs of tidal interactions or ongoing mergers. The overall shape is substantially rounded, with no noticeable elongation or asymmetry.
