The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, exhibiting a generally rounded morphology. There is a bright central bulge that fades gradually outward, and a more diffuse halo, indicating a relatively evolved system. There is very faint evidence of a potential disk component, but there is very little to no spiral structure. The object presents a consistent color gradient, with a slight reddish hue in the center. There do not appear to be any signs of major mergers or tidal disturbances and only minor signs of disturbance, suggesting the galaxy has undergone a fairly stable evolution. Overall, the galaxy has a well-defined structure and a relatively uniform stellar population distribution.
