The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. It is elongated in shape, with a high degree of flattening. A bright central bulge is evident, with a gradual decrease in luminosity towards the outer regions. The color profile indicates a redder core, which becomes slightly bluer moving away from the center and along the major axis. There is no evidence of spiral arms, dust lanes, or active star formation regions within the visible light spectrum. Overall, the galaxy displays characteristics consistent with a passively evolving system.
