The galaxy presents as an elongated, cigar-shaped structure. It exhibits a relatively smooth, albeit somewhat indistinct, morphology. The central region displays a concentration of light, appearing as a yellowish-orange core, possibly indicating an older stellar population or dust obscuration. The outer regions of the galaxy transition to a more diffuse bluish hue, suggestive of younger stars or active star formation. There are some subtle irregularities in the light distribution, but no obvious signs of major disturbances or ongoing mergers.
