This galaxy appears to be a relatively smooth, elliptical galaxy, possessing a high degree of central concentration. The light distribution suggests a spheroidal morphology with minimal discernible features such as spiral arms or prominent dust lanes. The galaxy exhibits a notable color gradient, shifting from a bluer hue in the central region to redder colors towards its periphery. This could imply a centrally concentrated population of younger, hotter stars with older, cooler stars dominating the outer regions. The overall structure displays a moderate roundness, showing only slight deviations from a perfect circular shape. There is no strong evidence of any major ongoing merger activity or tidal disturbances. It is possible the object is a lenticular galaxy, but given the lack of a discernible disk, it is more likely an elliptical.
