The galaxy presents as a somewhat elongated, elliptical structure. The central bulge appears to be composed of older stellar populations, indicated by its yellowish color. The outer regions exhibit a fainter, more diffuse blue hue, suggesting the presence of younger, hotter stars. The overall shape suggests that the galaxy is more "in between" round or cigar shaped and is not likely a spiral. There are subtle indications of minor disturbances in the galactic structure, possibly a result of past interactions or minor mergers, however the structure is largely unperturbed. The galaxy appears to be in an intermediate stage of its life cycle, with moderate star formation activity occurring within its disk or outer regions.
