The galaxy presents as a somewhat diffuse, elliptical structure with a bright, concentrated central region. The core exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the galaxy displays a more bluish tint, indicative of younger stars. The overall form deviates from a perfect elliptical shape, showing signs of potential disturbance, which could be indicative of a past or ongoing interaction or merger event. Faint tidal features may be present, but higher resolution data would be needed to confirm the nature and magnitude of the event.
