The galaxy presents an overall elongated, cigar-like morphology. It displays a relatively smooth appearance, with a centrally concentrated bulge that exhibits a yellowish-orange hue, suggesting an older stellar population. The light diminishes gradually towards the outer edges of the galaxy, though there is a hint of a disk structure as there is a slight flattening of the galaxy. There is a relatively low level of disruption observed. The estimated mass of the galaxy is quite large, meaning the object is likely a giant galaxy. Overall, this galaxy appears to be relatively undisturbed, possessing a significant bulge and a smoothly fading disk.
