The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical with a high degree of roundness. There is no discernible disk structure or spiral arm features. The light distribution suggests a fairly uniform stellar population. The galaxy exhibits a color gradient, appearing slightly bluer in the central region and gradually becoming redder toward the outskirts. There are no obvious signs of major mergers or significant tidal disturbances. Faint, diffuse light extends outwards from the central region, blending into the background sky.
