The galaxy presents as a relatively compact, elliptical system. Its light profile appears smooth and centrally concentrated, lacking any obvious spiral arm structure or prominent dust lanes. The galaxy exhibits a yellowish-white hue, suggesting a population of older stars. The overall shape is close to circular, with only a very slight deviation towards ellipticity. No significant tidal features or signs of ongoing merger activity are discernible, implying it is a relatively undisturbed system. 
