The observed galaxy presents a roughly elliptical morphology with a moderate degree of central concentration. There is a bright, compact core. The color gradient is fairly uniform, shifting from a central yellowish hue to a bluer periphery. Faint distortions are visible within the central region, potentially indicative of minor gravitational interactions or internal dynamics. There appears to be a slight disturbance in the overall symmetry of the galaxy. The galaxy lacks prominent spiral arm structures or a well-defined disk component.
