The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with no discernible spiral arms or disk-like structure. It is characterized by a generally round shape. The light distribution suggests a high degree of central concentration, with the brightest region located at the core and a gradual decrease in luminosity toward the outer edges. The color appears predominantly yellowish-orange, which would be consistent with an older stellar population and low ongoing star formation. There is no visible evidence of dust lanes or recent merger events. It has a moderate redshift, suggesting it is at a considerable cosmological distance. Based on its smooth morphology and color, this galaxy is likely a relatively massive system.
