The galaxy presents as a smooth, elongated structure with a high degree of central concentration. It appears to be an elliptical galaxy viewed nearly edge-on. The galaxy exhibits a notable color gradient, with a yellowish central bulge region transitioning to bluer outer regions. There is no evidence of spiral arm structure, dust lanes, or ongoing major merger activity. The smooth and regular morphology suggests that this galaxy has undergone substantial dynamical relaxation and that star formation is likely suppressed. The absence of significant morphological distortions implies a relatively quiescent evolutionary history. The galaxy appears to be an isolated system, with no signs of a nearby companion that could be gravitationally interacting.