The galaxy appears as a relatively smooth and centrally concentrated object. The morphology is largely elliptical, exhibiting a moderate degree of roundness. There is a slight color gradient with a suggestion of bluer hues toward the central region, indicating potentially younger stellar populations in this location. No spiral arm structures or distinct disk features are discernible. There may be some indications of minor disturbances, as the galaxy is slightly asymmetrical, but it is difficult to fully assess with the image's resolution. The galaxy shows no strong evidence of major mergers or significant tidal interactions. The object is likely a massive galaxy with moderate star formation activity.