The galaxy presents a notably elongated, cigar-shaped morphology. It exhibits a smooth, relatively featureless profile, suggestive of an elliptical galaxy type. The central region displays a yellowish-orange hue, possibly indicating an older stellar population, while the outer regions show a subtle gradient towards a blueish-green tint. The overall color variation suggests a difference in stellar population or dust content across the galaxy. There is no readily apparent evidence of spiral arms or ongoing major mergers, though subtle disturbances cannot be ruled out with this image.
