The galaxy appears as a generally smooth, elliptical-like structure with a concentrated central bulge. The light profile suggests a relatively uniform distribution, becoming more diffuse in the outer regions, and a bright core that is slightly off-center. There is a subtle color gradient visible. The galaxy's core is characterized by a yellowish-white hue, which subtly transitions to a more reddish tone in its extended halo. There is no distinct disk visible, nor any prominent spiral arms. Faint irregularities in the outer regions suggest either tidal disturbances or minor interactions with smaller satellite galaxies, although the overall morphology is not significantly disrupted. Based on its apparent size and the observed redshift, this is likely a massive galaxy at a considerable distance. Given the morphology, the current rate of star formation is probably low.
