The galaxy exhibits a largely smooth morphology, with a high degree of central concentration. Its overall shape appears close to round, with a slight extension along one axis. The core region displays a bright, yellowish-white hue, suggesting a population of older stars or significant dust obscuration. Fainter, bluer light extends outwards from the core, possibly indicative of a disk or spiral arms. There is visual evidence of possible tidal disturbances or merger activity. The galaxy is most likely an elliptical galaxy with some unique characteristics.
