The galaxy appears to be a relatively smooth, elliptical-type galaxy. It presents with a concentrated, nearly spherical light profile, indicating a high degree of central mass concentration. The light is yellowish, suggesting an older stellar population, with less ongoing star formation. There is no apparent disk structure or spiral arms visible, further supporting its classification as an elliptical. Faint, diffuse outer regions are seen, but these lack discernible features or structure. There is no evidence of any active galactic nucleus or significant dust lanes within the galaxy's structure. The galaxy appears isolated, showing no obvious signs of tidal interactions or ongoing mergers with other galaxies.
