The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of luminosity, appearing bright and yellowish-orange. The isophotes fade gradually outward, suggesting a decreasing stellar density with increasing radius. There is some subtle color variation, hinting at potential differences in stellar populations or dust content. The overall morphology is consistent with an early-type galaxy, potentially an elliptical or S0, with no clear signs of spiral arms or significant disk features visible in this image. There is no strong evidence of tidal features or recent mergers, although subtle irregularities might be present upon closer inspection.
