The galaxy appears as an elongated, cigar-shaped structure, with an apparent axis ratio of roughly 5:1. The light distribution indicates a relatively smooth morphology, lacking prominent spiral arms or distinct features. Color gradients are present. The central region exhibits a yellow-orange hue, potentially indicative of an older stellar population. Fainter blue tinges are visible towards the extremities, suggesting the presence of younger, hotter stars, although they are not distinctly resolved. There is no obvious presence of significant dust lanes or active star-forming regions, although faint color variations may indicate subtle variations in stellar populations or dust content across the galaxy. The galaxy does not show any signs of major ongoing mergers or tidal disturbances. Overall, this galaxy appears to be a relatively quiescent system, consistent with an early-type morphology such as an elliptical or lenticular galaxy, observed at a significant distance.
