The galaxy presents as a central, bright, ochre-colored spheroid structure. A faint, diffuse, greenish-blue halo surrounds the bright core, extending outwards. There appears to be a slight flattening, suggesting it is not perfectly spherical. Irregularities within the halo indicate possible disturbances, such as minor gravitational interactions or active galactic nuclei outflow. There is no clear evidence of a disk or spiral structure; the morphology appears to be largely spheroidal and dominated by an old stellar population. The overall color profile suggests ongoing but potentially subdued star formation activity in the outer regions, with the central region being dominated by an older stellar population.
