The galaxy presents as a centrally concentrated, elliptical morphology. A smooth light profile dominates the visible structure, with no immediately apparent spiral arms or prominent disk features. The core region exhibits a bright, concentrated luminosity suggesting a high stellar density. The overall color profile is redder, hinting at a more evolved stellar population and potentially higher dust content. The galaxy exhibits an elongated shape with some features, but the lack of tidal tails or other signs of major disruption suggests it is not currently undergoing a significant merging event. There may be a degree of minor disturbance.
