The galaxy appears to be an elliptical type. It presents a smooth, concentrated light profile. The core region is a bright yellow to gold color, which may indicate the presence of an older stellar population. The galaxy exhibits a high degree of circularity. There appears to be no significant evidence of spiral arm structure or a prominent disk component. No significant tidal features or other signs of recent major merger activity are evident. There may be some very minor disturbances visible, or potentially faint artifacts in the image.
