The galaxy appears as a single, consolidated luminous entity. The core of the galaxy exhibits a distinct yellow-orange hue, indicative of an older stellar population dominating the central region. There is a notable decrease in luminosity from the central core outwards, suggesting a concentration of stellar density towards the center. The shape is not perfectly spherical; it is slightly elongated but falls predominantly into the "in between" category regarding roundness. There are no obvious signs of spiral arms or a well-defined disk structure visible at this resolution. It has a relatively smooth appearance with no signs of major ongoing mergers. It appears quite massive based on its luminosity. The blue color suggests there is evidence of some amount of ongoing, but low, star formation.
