The galaxy presents a generally smooth morphology with little discernible internal structure. Its light profile appears centrally concentrated, with a gradual falloff in intensity toward the outer regions. The primary color is a yellowish-orange hue, potentially indicating an older stellar population and a reduced rate of ongoing star formation. There is a slight asymmetry in the outer contours, with a hint of faint extension on one side, which might suggest a minor gravitational interaction or tidal disturbance, though it could also be due to projection effects or internal dust obscuration. Overall, the galaxy appears to be an evolved system, possibly an elliptical galaxy or a lenticular galaxy viewed at low inclination.
