The galaxy presents an overall elliptical morphology, exhibiting a smooth, diffuse light distribution. The core region is bright and concentrated, indicating a high stellar density. The outer regions gradually fade into the background, suggesting a decreasing stellar population density with increasing distance from the galactic center. There is a subtle color gradient, shifting from a yellowish-white hue at the center to a slightly redder tone in the outer regions. No distinct spiral arms or dust lanes are readily apparent. The overall structure appears regular, with no obvious signs of recent major mergers or tidal distortions. The shape of the galaxy is nearly circular, with a small amount of elongation.
