The galaxy presents a predominantly smooth morphology. It appears elliptical in shape, exhibiting a high degree of central concentration with a bright core. A faint, diffuse halo surrounds the central region. The color gradient shows a yellowish-white hue at the core, transitioning towards a greenish color as the distance from the center increases, hinting at potential variations in stellar populations or dust content. There is little evidence of spiral arms or significant disk structures, suggesting it may be an early-type galaxy. There is no obvious indication of any ongoing major merging activity, although subtle irregularities could indicate minor disturbances. The overall impression is of a relatively evolved and settled system.
