The galaxy presents a generally elliptical morphology, appearing relatively smooth with a highly concentrated central bulge. The light distribution suggests an older stellar population, with a yellowish-white hue dominating the inner region. Fainter, somewhat asymmetrical, blueish extensions are observed away from the core. The color gradients from the core outwards imply a shift from older, redder stars in the center to possibly younger, bluer stars within the surrounding regions. This suggests that the central regions are comprised of old stars whereas more recent and localized star formation may be occurring in other areas of the galaxy. There may be ongoing minor disturbances within the structure or some sort of interaction. Based on its apparent smoothness and roundness, it is likely an elliptical galaxy that has already exhausted most of its gas reservoir.