The galaxy presents as a relatively compact object, exhibiting an overall elliptical morphology. The central region displays a high degree of luminosity, suggesting a concentration of older stellar populations. A diffuse, less luminous halo extends outward from the core. Evident within the galaxy are multiple regions of differing color composition. One notable region exhibits bluer colors than the core, indicating a more recent episode of star formation. This region appears somewhat disturbed, showing signs that suggests a possible tidal interaction or merger event. The smoothness of the overall structure, combined with the presence of some disturbance, indicates a galaxy likely transitioning from a more active, irregular state towards a more quiescent, elliptical form.
