The observed galaxy presents a relatively smooth morphology, with a centrally concentrated light distribution. It appears largely elliptical in shape, but deviates slightly from a perfect ellipse, displaying a mild degree of intermediate roundness. There is a subtle elongation along one axis.

There is likely no major disk component visible. Evidence of merging is present, but not highly disruptive. Instead of a large major disruption in the system, there appear to be some possible signs of tidal interaction and a minor disturbance, with some hint of external structure in the halo.
