The galaxy appears to be a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge which appears to be yellow-orange in color, suggesting an older stellar population. The galaxy fades outwards from the center in all directions. There are no obvious spiral arm structures or significant dust lanes visible, nor is there evidence of any tidal tails or obvious signs of mergers. The galaxy is roughly circular in shape, with a slight elongation, but it appears fairly symmetrical overall. The outer regions exhibit a bluer hue. The isophotes appear relatively smooth and regular, indicative of a system that has undergone significant dynamical relaxation. The galaxy appears to be an evolved system with diminished star formation.
