The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated bulge, transitioning to a more diffuse halo. A subtle color gradient is observed; the core appears more yellow/gold, suggestive of an older stellar population, whereas the outer regions display a bluer hue, implying the presence of younger, hotter stars, albeit at a lower density. There are no prominent spiral arms or distinct dust lanes visible. The overall shape is slightly elongated. No signs of major disturbances or ongoing mergers are immediately apparent, with a smooth gradient transitioning from the center of the galaxy to it's outer edges.
