The galaxy presents as a single, elongated, cigar-shaped structure. Its light profile shows a concentration of luminosity toward the center, fading outwards. The core exhibits a reddish hue, suggesting an older stellar population or significant dust obscuration. Fainter, bluer light is observed on the outer edges, which hints at younger stars or active star formation there. The overall morphology appears relatively undisturbed, with no obvious signs of tidal features or major mergers.
