The galaxy presents a generally elliptical morphology, exhibiting a high degree of central concentration. The core region appears very bright and unresolved, indicating a significant density of stars. Extending outwards from the core, a fainter, more diffuse halo is observed. The halo appears relatively smooth with a slight flattening along one axis, suggesting a possible elliptical shape. There is an indication of a potential minor disturbance, with a slight asymmetry noted in the halo's outer regions, giving a possible sign of a small scale merger occuring. Overall, the galaxy appears relatively quiescent and evolved.
