The galaxy presents as a centrally concentrated structure with a generally smooth appearance, suggesting an elliptical morphology or a spiral galaxy viewed face-on with a dominant bulge. It exhibits a yellowish-orange hue, which could indicate an older stellar population with fewer young, massive stars. The galaxy appears fairly symmetrical with a high degree of central concentration. There is no obvious spiral arm structure or dust lane. The light distribution falls off gradually from the core, with a small change in color as the radius increases. The galaxy appears to be an isolated object, without obvious signs of interaction or disturbance. There is no evidence of active star formation.
