The galaxy presents as a centrally concentrated object, likely an elliptical. There is a high degree of smoothness to the overall light distribution, with little evidence of spiral arm structure or dust lanes. The central region exhibits a yellow-orange hue, which could indicate an older stellar population dominating this area. The outer regions fade into a fainter blueish color, suggesting a younger population of stars may be sparsely distributed further out. The isophotes appear largely regular and elliptical, though there may be a slight tidal tail or other disturbance on one side. Overall, this galaxy presents as a relatively evolved and quiescent system.
