The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. The core region exhibits a concentrated, bright intensity, transitioning outwards to a more diffuse, less luminous halo. There is a subtle color gradient, with the central bulge appearing slightly redder than the outer regions, which exhibit a hint of greenish-yellow. The galaxy's overall shape is mostly circular, with no apparent spiral arm structures or major morphological disturbances. There might be a very faint, extended halo surrounding the main body of the galaxy, though this is difficult to discern due to image noise. No distinct dust lanes or significant star-forming regions are clearly visible. The overall appearance suggests a mature galaxy with a significant population of older stars and relatively low current star formation activity.
