The galaxy presents a morphology that appears largely smooth and elliptical in shape. There is some indication of a slight disc structure. The galaxy exhibits a color gradient, shifting from a redder hue at its core to a slightly bluer color in the outer regions. This suggests a higher concentration of older stellar populations towards the center, and possibly younger, star-forming regions further away. The overall appearance indicates an evolved system, potentially in the process of quenching star formation. Weak disturbances may be present; however, a significant merger event is unlikely. The galaxy's light profile is relatively concentrated.
