The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards its outer edges. The light distribution suggests it is mostly spheroidal in shape, with very little evidence of spiral arms or a well-defined disk component. The galaxy's color is primarily a pale blue-white hue in the central region, with some evidence of redder colors along the edges. There are no obvious signs of significant ongoing star formation within the galaxy based on its color and morphology. The overall impression is that of a mature, relatively undisturbed system. The galaxy appears largely isolated, without obvious signs of interaction or recent merger events.
