The galaxy presents as an elliptical morphology with a smooth, diffuse appearance. Its core exhibits a concentrated luminosity gradient, suggesting a high stellar density in the central region. The overall color profile is indicative of an older stellar population, with a yellowish hue dominating the galaxy's light. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears relatively undisturbed, without any obvious signs of recent major mergers or tidal interactions. A slight asymmetry is observed in the outer halo. The size of the galaxy, while not explicitly resolved, appears moderately large, further supporting classification as a large elliptical galaxy. The apparent magnitude suggests it is a luminous object at its given redshift. The inferred low star formation rate is consistent with the older stellar population implied by the color and morphology.
