The object presents as an elongated, cigar-shaped galaxy. Its color profile suggests an older stellar population dominating its composition, with a noticeable redder hue throughout. While the image lacks the resolution to resolve individual stars or dust lanes, there is a smoothness to its overall appearance. The galaxy appears relatively undisturbed, with no obvious signs of ongoing mergers or tidal interactions. The brightness distribution gradually decreases from the central region outwards, indicating a concentrated core.
