The galaxy appears as a centrally concentrated, luminous object. The core exhibits a yellowish-orange hue, suggesting an older stellar population. Moving outward from the center, the light gradually transitions to a fainter, diffuse white, indicating the presence of younger stars and potentially ongoing star formation in the outer regions, but at a seemingly lower rate than observed in typical starburst galaxies. The object presents an elliptical shape with a round appearance; the smooth, even light distribution suggests a lack of major structural disturbances, such as spiral arms or tidal tails. The galaxy appears relatively isolated, showing no obvious signs of recent or ongoing major mergers with other galaxies. It is a relatively massive galaxy, given its apparent luminosity at its redshift.
