The galaxy presents as a lenticular, or possibly an edge-on spiral, system. The light distribution appears relatively smooth, with a concentration towards the center. The elongated morphology gives it a cigar-like appearance. There are faint signs of possible disturbances in the disk, but no strong evidence of any ongoing mergers or major tidal interactions. Based on the color indices, there are signs of modest star formation activity, but is not dominated by young stellar populations. The system is relatively massive. Overall, the galaxy exhibits a moderate redshift, indicating an appreciable distance.
