The galaxy appears as a smooth, elliptical-like object, displaying a relatively featureless morphology. Its color profile suggests a predominantly older stellar population, with a greater concentration in the redder bands of the visible spectrum, with slightly younger stars in the very center of the galaxy. The overall shape indicates a morphology somewhere between a sphere and a flattened ellipse. There is no discernible evidence of spiral arms or a prominent disk structure. The smoothness of the light distribution suggests that the galaxy has likely undergone significant dynamical relaxation and potentially lacks ongoing major star formation activity. There are subtle signs of disturbance in the edges of the galaxy, hinting at a possible past minor merger event.
