The galaxy exhibits a generally smooth morphology. It has a largely elliptical shape, with a high degree of roundness. The galaxy's core appears bright and concentrated. There are no prominent spiral arms or distinct features indicative of ongoing disk formation. The light distribution is relatively smooth, which is potentially indicative of an older stellar population. Faint disturbances or irregular features hint at possible past interactions or merger events. The galaxy's color suggests a dominant population of older stars with a low current star formation rate. This galaxy appears to be undergoing, or has undergone, a merging event.