The galaxy presents as a relatively smooth, elliptical-like structure with a moderately elongated shape. There is a concentration of light towards the central region, suggesting a bulge or a dense nucleus. The overall color appears bluish, possibly indicating a population of younger, hotter stars, but this interpretation requires careful consideration due to potential redshift effects. Faint color variations may exist in the central regions. No distinct spiral arms or obvious dust lanes are apparent in this image, suggesting a lack of significant recent star formation or organized structure. There are no signs of major mergers or significant tidal disturbances, though the possibility of minor past interactions cannot be ruled out based on this image alone.
