The galaxy presents as an elongated, cigar-shaped structure. It exhibits a relatively smooth morphology with a slight central concentration of light. The color profile suggests a redder hue, potentially indicating an older stellar population or significant dust obscuration. There's no obvious presence of spiral arms or strong star-forming regions. The galaxy appears isolated, with no immediately apparent major mergers or tidal disturbances, although minor disturbances cannot be ruled out. It's classified as a disk galaxy, but is likely a smooth variant.