The galaxy presents a largely smooth morphology, exhibiting a high degree of central concentration. The light profile suggests an elliptical or lenticular classification. There is a distinct color gradient, transitioning from a redder core to bluer, less concentrated outskirts. There is no apparent spiral arm structure or significant dust lane obscuration. No features of tidal disturbance, or evidence of an ongoing major merger are visible, though a minor interaction cannot be ruled out completely. The galaxy appears approximately round in shape. The overall color suggests an older stellar population. It is a relatively massive galaxy, with a moderate rate of star formation.
