The galaxy presents as a relatively small, faint, and elongated structure. Its light is predominantly a smooth, blue-white hue, suggesting a relatively old stellar population. The lack of distinct spiral arms or prominent features implies a morphology closer to an elliptical or lenticular galaxy. The smooth light distribution indicates that any ongoing star formation is subdued. There is minimal evidence of significant dust lanes or patchy star formation regions. The galaxy appears largely undisturbed, without indications of major mergers or tidal interactions. The cigar-like shape suggests it may be a somewhat flattened system or is viewed at an angle. The overall appearance suggests a stable, relatively quiescent galaxy, with little recent activity.
