The galaxy presents a smooth, elliptical morphology, exhibiting a centrally concentrated luminosity profile. The core region displays a yellowish-white hue, suggesting an older stellar population dominates this area. Moving outward from the core, there is a subtle transition towards bluer tones, hinting at the presence of some younger, hotter stars.

The galaxy appears somewhat elongated, with a slight cigar-shaped structure. Evidence of significant disk-like features or spiral arms is absent, supporting its classification as an elliptical galaxy. No significant signs of major mergers or tidal disturbances are apparent in this image, indicating that this galaxy is not currently undergoing a major interaction. Minor asymmetries or disturbances cannot be ruled out, but they do not dominate the overall structure.
