The galaxy presents as an elongated, cigar-shaped structure with a smooth, relatively featureless appearance. It exhibits a color gradient, with a brighter, more concentrated yellowish-white central region, suggestive of an older stellar population or dust obscuration. The outer regions appear fainter and exhibit a subtle bluish tinge, hinting at a younger stellar population or ongoing star formation. There is no evidence of spiral arms, bars, or significant dust lanes. The overall morphology appears undisturbed, with no clear signs of tidal interactions or recent mergers. The galaxy's profile suggests it is likely an edge-on or highly inclined disk galaxy or potentially an elliptical galaxy. Its apparent angular size is relatively small, implying either a modest physical size or significant distance.
