The galaxy presents as a single, relatively smooth object with a high degree of central concentration. It appears nearly circular in projection, suggesting it could be an elliptical galaxy or a face-on spiral with a dominant bulge. The galaxy exhibits a subtle color gradient, appearing slightly bluer towards the outer regions and redder in the central core, which may indicate differing stellar populations or dust distribution. There is no discernible evidence of a disk structure, spiral arms, or significant tidal disturbances. Overall, the galaxy presents as a mature system with little to no ongoing major merger activity.
