The galaxy presents as a relatively smooth, elliptical structure, exhibiting a central, concentrated bulge with a somewhat diffuse halo. There is a slight elongation in the shape, being somewhere between round and cigar shaped, but overall is smooth. The color gradient is subtle, with the core appearing slightly bluer than the outer regions. There are no immediately apparent spiral arms or significant dust lanes visible. The lack of discernible features suggests a more evolved stellar population with relatively low ongoing star formation. There is no indication of a major merger occurring. There could be signs of minor disturbance, but it is difficult to discern at the current resolution. The overall appearance indicates a considerable mass, characteristic of an elliptical galaxy at a non-negligible redshift.
