The galaxy presents a largely smooth and centrally concentrated morphology. It appears elliptical in shape, exhibiting a high degree of circularity. The light profile suggests a bulge-dominated system, with a gradual decline in luminosity from the center outwards. The galaxy has an apparent color gradient, being yellower towards the core and exhibiting slight blueing in the outer regions of the galaxy. There is no evidence of spiral arms, a prominent disk, or any ongoing major merger activity. The galaxy's structure appears relatively undisturbed, showing only minor irregularities. Given the observed morphology, it's likely a massive galaxy with a low specific star formation rate.
