The galaxy presents as a relatively face-on system, exhibiting a smooth, elliptical morphology with a central, highly luminous bulge. There is little evidence of spiral arm structure or significant dust lanes. The overall color is a pale yellow, which likely implies a stellar population dominated by older, less massive stars. The light distribution appears relatively uniform, with the intensity decreasing gradually from the bright central bulge to the outer regions of the galaxy. The relatively high concentration of light towards the center indicates a high Sersic index, suggesting an elliptical galaxy type. There is a subtle color gradient from the center to the outer edges, where the color seems to lean more towards the blue spectrum. This system looks to be undisturbed, not showing any morphological signs of recent mergers or interactions.