The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of central concentration. The galaxy's color profile is dominated by a yellowish-white hue in the core, with a faint redder periphery, indicative of an aging stellar population and reduced star formation activity. There is no clear evidence of spiral arm structure or a distinct disk. The shape appears almost perfectly round. Possible slight disturbances exist in the outer areas of the galaxy. No clear signs of major mergers are present.
