The galaxy presents as an elliptical structure with a smooth light distribution, exhibiting no discernible spiral arms or significant dust lanes. Its morphology appears to be intermediate between a perfectly circular and a highly elongated shape. The central region shows a concentration of light, suggesting the presence of a bulge component. The outer regions fade gradually into the background, indicating a smooth stellar halo. There is a slight asymmetry or minor disturbance on one side of the galaxy, suggesting a possible interaction or minor merger history. The overall color is predominantly yellow-white, implying a population of older stars with relatively low ongoing star formation.
