This galaxy presents as a relatively compact object with a disturbed morphology. The central region exhibits a high surface brightness, appearing bright white and slightly extended. A diffuse, blue halo surrounds this bright core, suggesting the presence of younger, hotter stellar populations. There is a prominent, irregular feature to one side of the central region, displaying a darker, possibly obscured region adjacent to it. The overall color distribution points to an ongoing or recent interaction or merger event disrupting the galaxy's structure, and shows signs of star formation within the brighter areas.
