The galaxy appears to be a single, relatively smooth object with a somewhat elliptical morphology. It presents a yellow-orange hue, indicating an older stellar population and potentially lower ongoing star formation. There is a slight deviation from perfect circularity, appearing more "in between" of round and cigar shaped, but it is predominantly smooth and well-defined. There are no obvious signs of major mergers or significant disturbances in its structure. The galaxy's light is relatively concentrated, suggesting a high degree of central mass concentration. There are no visible spiral arms, bars, or dust lanes.
