This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing significantly brighter and more yellow/orange than the outer regions, suggesting an older stellar population. The overall shape is elongated, but not dramatically so, tending toward a more spheroidal form. There is a slight hint of bluer light in the outer edges, potentially indicating some ongoing, albeit limited, star formation in the disk. The galaxy does not appear to be undergoing any major merging events or showing strong tidal disturbances, although there is some very minor asymmetry that could point to the remains of a past interaction. The light is relatively concentrated suggesting this is a pretty massive galaxy.
