The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. It appears to be relatively round in shape. There is a distinct color gradient, transitioning from a blueish hue in the lower region to a more golden hue in the center, and a redder hue in the surrounding region. This suggests potential variations in stellar populations or dust content across the galaxy. There may be an interaction or merger occurring, given the irregular extensions or distortions in the central regions. The stellar mass appears to be substantial, indicative of a mature system. The star formation rate appears to be suppressed.
