The galaxy presents as an elliptical structure, exhibiting a smooth, relatively featureless morphology. The central region displays a concentrated brightness, indicating a prominent galactic nucleus. A gradual decline in luminosity is observed extending outward from the core, suggesting a spheroidal distribution of stars. There is evidence of a subtle color gradient from a yellower core to more greenish outer regions. The overall structure exhibits a high degree of symmetry. No signs of significant tidal disturbances or ongoing merger events are apparent. The absence of distinct spiral arms or prominent dust lanes further supports its classification as an elliptical galaxy.
