The galaxy exhibits a primarily smooth morphology. There is a bright, compact central region that appears nearly spherical, suggestive of a significant bulge component or possibly an active galactic nucleus. Surrounding the bright core is a diffuse halo of light. The radial color profile indicates a color gradient, transitioning from a bluer hue in the inner regions to redder tones in the outer parts of the halo. This color variation may indicate differences in stellar populations, dust content, or star formation activity across the galaxy. Visual inspection suggests some asymmetry or possible tidal features emanating from the central body, hinting at a possible recent or ongoing merger event.
