The galaxy presents as a smooth, elongated, cigar-shaped structure. There is a central, brighter region with a yellow-white hue, suggesting an older stellar population or a concentration of dust. Fainter, bluer material extends outwards from the center, indicative of possible star formation in a disk-like structure. The overall morphology is relatively undisturbed, with no obvious signs of a major merger, although minor disturbances cannot be ruled out.
