This galaxy appears to be a relatively smooth, elliptical galaxy. It has a concentrated, bright core that fades gently into the surrounding halo. The galaxy appears fairly round in shape, with only a slight deviation from perfect circularity. There is no apparent disk structure or spiral arm morphology. There are no signs of ongoing major mergers or significant tidal disturbances. It exhibits a relatively uniform color gradient from the core to the outer regions, suggesting a somewhat homogenous stellar population.
