The galaxy appears to be a relatively large, smooth elliptical galaxy with a yellowish hue. It exhibits a high degree of central concentration, with the luminosity decreasing gradually from the core outwards. There is little evidence of spiral arms or significant dust lanes. The overall structure suggests an older stellar population, consistent with a passively evolving system. The galaxy displays a slightly elongated shape, but overall seems well ordered. No signs of active galactic nuclei-related jets are apparent. While the core of the galaxy is bright, there are no obvious signs of recent mergers or major disturbances in the system's morphology, although subtle asymmetric features cannot be ruled out due to image resolution.
