The galaxy appears roughly circular in shape, with a relatively smooth and featureless central bulge. The color distribution indicates a possible gradient, shifting from a bluer hue in the center to a more reddish tinge towards the outer regions. The presence of the bluer core suggests potential ongoing star formation activity within the central region of the galaxy. There may be minor disturbances or a potential merging event interacting with the galaxy, leading to the irregular shape and the uneven distribution of light. It is difficult to discern definitive spiral arms or other complex structures. Overall, this galaxy seems to be in a transitional stage, possibly evolving from a more active, star-forming system to a more quiescent elliptical morphology.
