The galaxy presents as a somewhat elliptical, though not perfectly spherical, luminous object. Its color profile appears to be dominated by warmer hues, trending towards the redder end of the spectrum. The central region is noticeably brighter and more concentrated, suggesting a higher density of stars in the galactic nucleus or core. The outer regions fade gradually, indicating a decreasing stellar density with increasing distance from the center.  There is faint evidence of a possible disk structure. No strong evidence of recent major merging events or significant tidal disturbances is apparent in this image. The overall structure appears relatively settled and evolved.
