The galaxy presents as a generally elongated object, with a cigar-shaped morphology. A bulge is implied by a concentration of light towards the center of the galaxy. A disk component is also indicated. The galaxy displays a generally smooth appearance, with some areas showing disturbance. There are some indications of faint irregularities in the disk, with minor asymmetries suggesting some gravitational interaction or internal processes affecting the galaxy's structure. The color profile reveals a yellow-orange hue toward the central region that shifts to a blue-green tint in the outer areas, suggestive of differing stellar populations or dust content across the galaxy.
