The galaxy presents a relatively smooth and concentrated morphology. It exhibits a slightly elliptical shape, deviating marginally from perfect circularity. Color gradients are noticeable, with a bluer, potentially star-forming core region transitioning to redder hues in the outer regions. The central region is particularly bright and compact, indicative of a high stellar density. There is no clear evidence of spiral arms or a distinct disk structure in this image. While the overall structure appears relatively undisturbed, there may be a very minor asymmetry or irregularity in the outer regions, suggesting a possible past interaction or minor disturbance.
