This galaxy appears to be a relatively smooth, elliptical-type system, exhibiting a high degree of central concentration. The galaxy displays a somewhat spherical shape, with the isophotes appearing mostly round, without strong evidence of a disk component. There's a distinct color gradient, trending from a bluer hue in the outer regions toward a more yellow-red core. This could indicate an older stellar population concentrated in the galaxy's center, possibly a supermassive black hole. There are no obvious signs of recent major mergers or significant tidal disturbances, but subtle features might be present at a lower contrast level. Overall, it appears to be a quiescent system, without pronounced star formation regions.
