The galaxy presents a generally smooth and rounded morphology. It appears to be an elliptical galaxy with a bright, concentrated central region, likely representing a significant bulge component. Fainter and more diffuse light extends outwards from the core. There is no readily apparent spiral structure, disk, or significant dust lanes. The light emitted by the galaxy is relatively even in color, with yellow/white tones in the core, transitioning to slightly redder hues in the outer regions. There is no visible evidence of major mergers, tidal tails, or other strong gravitational disturbances. The overall appearance suggests a relatively evolved system with a largely quiescent stellar population.
