The galaxy presents as a slightly elongated, elliptical form. Its light is generally smooth and centrally concentrated, indicating an older stellar population. There appears to be very little evidence of spiral arm structure or significant dust lanes. Color gradients are subtle; the core exhibits a slight yellowish hue, while the outer regions are tinged with blue. This suggests some ongoing, albeit limited, star formation. The light appears to be relatively consistent and there are no signs of strong tidal features or a recent merger, the outer region looks to be quite smooth. The galaxy overall appears to be relatively quiescent.
