The galaxy presents as a smooth, elongated structure with a cigar-like shape. It exhibits a predominantly red color, potentially indicating an older stellar population and reduced star formation activity. The central region appears brighter and more concentrated, suggesting a nucleus. There is minimal evidence of spiral arms or disk-like features. The overall morphology suggests an elliptical galaxy, possibly of type E4-E7 given its significant elongation. There are no obvious signs of major disturbances or ongoing mergers.
