The galaxy appears to be a relatively smooth, elliptical galaxy with a centrally concentrated brightness profile. There's a distinct core region that seems to be reddish in color, suggesting an older stellar population. Surrounding the core, there's a fainter, more diffuse halo of light that extends outwards. This halo exhibits a bluer color, hinting at a younger stellar population or possibly some ongoing star formation, albeit at a low rate. There is no distinct spiral arm structure or strong signs of dust lanes evident in the image. The overall appearance indicates the galaxy is fairly relaxed and not currently undergoing a major merger event, though there is some indication of minor disturbances. The galaxy's shape appears somewhat rounded.
