The galaxy presents as a single, relatively smooth object with an elliptical morphology. It exhibits a high degree of central concentration, with the luminosity appearing brightest at the galactic center. Moving outward from the center, the brightness smoothly decreases without any distinct spiral arm structures or prominent star-forming regions visible. There is an apparent absence of dust lanes. The galaxy is slightly elongated and has a stellar mass around 10^10 solar masses. The galaxy appears to be undergoing relatively little star formation at present. No significant tidal disturbances or signs of recent merger activity are clearly visible.
