The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification, though subtle features hinting at a possible disk component are present. It displays a moderate degree of roundness, appearing neither perfectly spherical nor significantly elongated. The galaxy exhibits a color gradient, transitioning from bluer hues in the central region to redder tones in the outer areas. This color distribution suggests a central concentration of younger, hotter stars with older, cooler stars dominating the outskirts. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the image, although subtle asymmetries may indicate minor interactions or past events. The estimated effective radius of the galaxy is approximately 8.3 kiloparsecs. The galaxy's colors indicate that it is a relatively luminous object. Based on the available evidence, the galaxy is likely a massive, relatively evolved system, possibly undergoing a gradual decline in its star formation rate.
