The galaxy presents as a relatively smooth, elliptical structure. There is a noticeable color gradient, with the central bulge exhibiting a yellowish-orange hue suggestive of an older stellar population dominated by evolved stars. The outer regions appear slightly bluer, possibly indicating the presence of some younger, hotter stars, albeit in lower proportion to the older population. The galaxy is elongated, appearing somewhat cigar-shaped, with no prominent spiral arms or disk-like features immediately apparent. There seems to be a slight irregularity in its overall shape, possibly indicating past minor interactions or disturbances, but the core morphology remains largely undisturbed. No signs of major ongoing merger activity are readily visible.
