The galaxy presents as a largely featureless elliptical galaxy with a smooth light distribution, appearing almost spherical in shape. The light is concentrated towards the center, where it exhibits a bright, yellowish hue. There is a radial color gradient, with the central region trending toward warmer colors, suggesting an older stellar population. Fainter, bluish light extends outwards from the core, encompassing a larger radius, which may represent a younger, though still diffuse, stellar population. No prominent spiral arms, dust lanes, or other distinct morphological features are discernible. There is no apparent evidence of ongoing or recent major mergers or tidal disturbances. Minor irregularities in the outer isophotes may indicate minor interactions.
