The galaxy presents a largely smooth morphology with an elliptical shape. The core of the galaxy exhibits a high concentration of light, appearing almost spheroidal and gradually fading outwards. The galaxy is slightly flattened, but retains its overall elliptical shape. The color gradients are subtle, with the central region presenting a bluer hue, possibly indicating the presence of younger stellar populations or a weak active galactic nucleus. There's very little evidence of spiral arm structure or significant dust lanes. The absence of any prominent tidal features suggests that this galaxy has not undergone any recent major mergers. It appears to be a relatively isolated system.
