The galaxy appears to be a relatively smooth and centrally concentrated system. It exhibits a fairly elliptical morphology, but is nearly round. There is a bright, concentrated core which fades outwards into a diffuse halo or bulge. The galaxy presents a subtle color gradient, with the core appearing more yellowish or golden, suggesting an older stellar population dominating the central region. Fainter bluish hues can be seen in the outer regions, suggesting ongoing or recent star formation there, although not very strong. There are no obvious signs of spiral arms or a prominent disk. No major mergers or tidal disturbances are apparent from the image. The overall appearance suggests it may be an early-type galaxy with a moderate stellar mass, but it still has some ongoing star formation in its outskirts.
