The galaxy presents an elliptical morphology, appearing predominantly smooth with a high degree of roundness. A central bulge exhibits a strong concentration of light, indicating a high stellar density in that region. The galaxy displays a color gradient, with a yellowish hue in the core transitioning to redder tones in the outer regions. This color profile suggests an older stellar population and a lack of significant recent star formation. Minor asymmetry is observed, possibly indicative of a past interaction or disturbance, but no major merging events are apparent. The overall structure appears relatively undisturbed. The galaxy is a considerable distance away given its redshift.
