The galaxy presents as a largely smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, golden-hued luminosity that diminishes gradually towards the outer regions. The surrounding halo appears relatively uniform with no prominent spiral arm structures or distinct features such as dust lanes. The object presents as highly rounded in shape. There are no obvious signs of any major disturbances or ongoing mergers. There is a slight color variation from the core to the halo indicating differing stellar populations.
