The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical morphology. The light is concentrated towards the center, indicating a dense core. There is a noticeable decrease in luminosity as the radius increases from the central bulge. No distinct spiral arms or prominent dust lanes are observed. The overall color is yellowish-white, suggesting an older stellar population. The isophotes appear relatively circular, further supporting its classification as an elliptical galaxy. No signs of recent or ongoing mergers are visibly apparent, indicating a dynamically stable system.
