The galaxy presents a generally smooth morphology, appearing somewhat elliptical in shape. Its central region exhibits a bright, concentrated luminosity, trending towards a reddish-orange hue, possibly indicating an older stellar population. The outer regions display a gradual decrease in intensity, with a hint of bluer tones mixed in, suggesting the presence of some younger stars or active star formation, albeit not prominently. There is a slight elongation visible, hinting at a possible disk-like structure or a triaxial shape. No major disturbances or signs of ongoing mergers are immediately apparent, although subtle irregularities in the outer halo luminosity suggest a potential minor interaction in its past. The overall form doesn't appear perfectly round, but rather moderately elongated.
