The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a distinct, bright core region which dominates the overall luminosity. The luminosity appears to decrease gradually from the core outwards. The galaxy's color exhibits a general yellowish-white hue, possibly indicating an older stellar population, and a lower rate of ongoing star formation. There is a slight elongation to the overall shape, but it appears mostly circular when viewed from our observational perspective. No prominent spiral arms, dust lanes, or other features indicative of disk galaxies are discernible. No signs of major mergers are observable.
