The galaxy presents as a centrally concentrated structure with a largely smooth morphology, indicating it is likely an elliptical or lenticular type. The object exhibits a relatively round shape. There is a subtle indication of a minor disturbance or interaction, which is exhibited by a slightly elongated shape. The galaxy appears to be a relatively massive system with an ongoing, albeit subdued, level of star formation. The light from the galaxy appears to skew towards redder wavelengths, as evidenced by the relative brightness in the redder bands.
