The galaxy presents an overall elliptical morphology, exhibiting a smooth light distribution with a centrally concentrated bulge. There is faint evidence of a disk structure, but the smoothness of the light suggests this is not a very pronounced disk. The central region shows a yellow color, indicative of an older stellar population. Moving outward from the center, the color shifts toward a bluish hue, possibly signifying younger stars in these regions, and a faint hint of on-going star formation. Some minor irregularities in the outer regions are evident, possibly due to a minor gravitational disturbance, or tidal interaction with another galaxy. The lack of very clear structures indicates that this is likely a relatively evolved system.
