The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the color transitions to a faint greenish tint, possibly indicating some ongoing, albeit subdued, star formation activity. The overall shape is somewhat elongated but largely rounded. No distinct spiral arms or significant dust lanes are visible. The galaxy appears undisturbed, showing no strong signs of recent or ongoing mergers or interactions. The outer regions gradually fade into the background, denoting a smooth density gradient.
