The galaxy appears as an elliptical-shaped structure, with a smooth, centrally concentrated light distribution. The core is a bright, yellowish hue, suggesting an older stellar population. The galaxy's light profile gradually diminishes from the center outwards, with a relatively compact size. There is a noticeable lack of distinct spiral arms or prominent dust lanes. The overall morphology indicates a relatively evolved system. There are no obvious signs of recent major merger events, though a minor disturbance cannot be ruled out based on this image alone. The observed color and smooth structure suggest a galaxy where star formation is either suppressed or has ceased.
