The galaxy presents as a relatively smooth, centralized object. The core region exhibits a strong concentration of light, appearing yellowish-white, suggesting a population of older stars. Moving outwards from the core, there's a diffuse halo of bluer light, indicating the presence of some younger stars and potential star formation activity. The overall shape tends towards being round, without a strong disk component being apparent. There are no obvious signs of major tidal disturbances or ongoing mergers, though some subtle irregularities in the outer regions cannot be entirely ruled out as minor disturbances.
