The galaxy presents as an elliptical morphology, with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, indicating the presence of an older stellar population. Moving outward from the center, the light gradually diminishes, transitioning to a reddish-orange color, possibly due to dust attenuation or a change in the stellar population. No distinct spiral arms or features are readily apparent within the galaxy. The galaxy shows a slightly elongated shape. A lack of any notable disturbances suggests the galaxy is relatively undisturbed and is not undergoing a major merger.
