The galaxy appears as a slightly elongated, elliptical-like structure with a smooth, relatively featureless profile. There is a noticeable color gradient; the central region exhibits a yellowish-orange hue, possibly indicating an older stellar population. Moving outwards from the center, the galaxy transitions to a slightly bluer color, hinting at the presence of younger stars or regions of ongoing star formation in the outer areas, though these are not clearly resolved. The overall smoothness suggests a lack of significant dust lanes or spiral arm structures. The shape is not perfectly circular, showing a slight elongation which implies it may be more disk-like than a typical elliptical galaxy. There are no obvious signs of tidal disturbances or mergers, and the galaxy appears largely undisturbed.
