The galaxy appears to be a relatively smooth, elliptical galaxy. There is a concentrated central bulge exhibiting a reddish-orange hue. The outer regions of the galaxy display a subtle bluish tint, suggesting the presence of a younger stellar population compared to the core. The overall structure seems undisturbed, without any significant signs of tidal interactions or ongoing mergers. The galaxy's round morphology is evident, with a high degree of circular symmetry. There is little evidence of distinct spiral arms or a prominent disk.
