The galaxy presents a generally smooth morphology, with a slight elongation in its overall shape. The central region appears brighter and more concentrated, transitioning outwards to a more diffuse halo. While the galaxy is largely smooth, subtle distortions are noticeable, hinting at possible tidal interactions or internal dynamics. The color gradient suggests variations in stellar populations, with a more reddish hue in the central regions, potentially indicative of older stars, and bluer tinges in some of the outer regions, possibly indicating regions of more recent star formation. There is no clear spiral structure evident, so the galaxy is likely an elliptical or lenticular galaxy. There seems to be some minor dust or gas obscuring some regions, possibly due to a recent interaction. The overall light profile suggests that the galaxy is relatively massive.
