The galaxy appears as a somewhat smooth, elliptical-like structure. The central bulge is a concentrated region of yellowish-white light, suggesting a high density of older stars. Fainter, bluer hues are visible in the outer regions, indicative of some younger stellar populations and possibly ongoing, though relatively subdued, star formation. There are subtle hints of a disk-like structure, although the smooth appearance suggests it may be more akin to a lenticular galaxy. No prominent spiral arms or significant dust lanes are readily apparent. There are no signs of any major disturbances or mergers.
