The galaxy presents as a somewhat elongated, elliptical structure, with a smooth appearance, lacking prominent spiral arms or a distinct bulge. There is a subtle color gradient, suggesting a slightly bluer central region that fades towards a redder outer halo, consistent with ongoing or recent star formation concentrated in the core. The overall morphology implies a galaxy that is transitioning, or has already transitioned, into an elliptical type with a relatively moderate stellar mass and modest current star formation rate. The galaxy does not display any obvious signs of a major ongoing merger event, but minor disturbances cannot be completely ruled out due to the faintness of the galaxy. The galaxy appears to be moderately luminous.
