The galaxy appears as a relatively smooth, centrally concentrated object. The shape is somewhat elliptical, appearing more elongated than circular, but not extremely so. A central bulge is discernible, exhibiting a yellowish-white hue, suggesting an older stellar population. Surrounding the core, a fainter, bluer halo is visible. This halo may indicate the presence of younger stars or ongoing star formation, though the color is not intensely blue. There is no strong evidence of spiral arm structure or significant dust lanes. The overall appearance suggests a galaxy that has largely completed its major mergers, with only minor disturbances visible in the outer regions.
