The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge with a diffuse halo extending outwards. The color gradient suggests a population of older stars, exhibiting redder hues overall. There are no obvious spiral arm structures or dust lanes visible in the image. There is a slight hint of blue near the center, although it appears to be older and more evolved. It exhibits low star formation activity. There is no indication of any major mergers, though the possibility of a minor disturbance cannot be ruled out entirely. The galaxy appears to be generally undisturbed with a mostly spheroidal shape.
