The galaxy appears to be an elliptical galaxy with a smooth, cigar-shaped morphology. There is a concentration of light towards the center, suggesting a bright galactic nucleus. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a fainter, reddish-orange halo. This could be due to differing stellar populations, dust distribution, or redshift effects across the galaxy. The galaxy's light is not uniformly distributed, hinting at variations in stellar density and possibly recent or ongoing merger activity.