The galaxy presents as an elongated, cigar-shaped structure. Its luminosity suggests a substantial mass. A dominant central bulge is subtly visible, which fades into the outskirts of the galaxy. The galaxy exhibits a primarily smooth texture, with a slight hint of a disk-like component that might be responsible for the elongation. Possible minor disturbances or interactions are not overtly clear in this image, although the shape is not perfectly uniform. The color distribution suggests it is composed of a blend of stellar populations.
