The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that emits strongly, suggesting a high density of stars in the galactic nucleus. The overall color profile indicates a relatively evolved stellar population, trending toward redder hues. There is little evidence of spiral arm structures or significant dust lanes within the galaxy. The galaxy is largely undisturbed, displaying no clear signs of ongoing or recent major mergers. The galaxy exhibits a very slight elongation.
