The object presents as an elongated, cigar-shaped galaxy. A smooth, relatively featureless central bulge dominates the morphology. The color profile indicates an older stellar population, with a pronounced reddish hue concentrated in the bulge. Fainter, greenish-tinged features are present at the periphery, potentially indicative of younger stars or ongoing star formation. No strong evidence of spiral arms is apparent, suggesting a later-type spiral or an elliptical morphology. There are no obvious signs of major mergers or tidal disturbances, though some minor irregularities could point to past interactions. The galaxy appears relatively isolated.
