The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a high degree of central concentration of light, appearing nearly spheroidal. There is a noticeable color gradient, with the central region displaying a yellowish-white hue, suggestive of an older stellar population. Fainter, reddish-tinged outer regions hint at the presence of a more evolved stellar population extending beyond the bright central core. The overall light distribution is largely symmetric. There may be evidence of a very small disk like structure and/ or merger activity in the galaxy due to the apparent distortion of the shape from perfectly circular. Although, this distortion could be the result of a tidal tail or interaction with another nearby galaxy or object. 
