The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggestive of a substantial stellar population or active galactic nucleus. The light appears yellowish-orange, indicating a lack of significant recent star formation, potentially composed of older, redder stars, although the color is most likely redshifted. There is no discernible disk or spiral arm structure within the galaxy's morphology. The light smoothly dissipates into the surrounding space without any noticeable disturbances or ongoing mergers. It maintains a compact shape without the appearance of tidal tails or lopsidedness, exhibiting a high degree of roundness. 
