The galaxy presents a predominantly smooth, elliptical morphology. Its color profile indicates a concentration of older stellar populations, emitting strongly in the redder bands of the spectrum. There is no visually discernible disk structure or spiral arm formation; the overall appearance is that of a relatively quiescent system. The galaxy exhibits a high degree of radial symmetry, appearing nearly circular in projection. There's no evidence of ongoing major merger events or significant tidal disturbances in its immediate vicinity, although a very minor asymmetry or faint feature might be present in one region. The galaxy’s core exhibits a high surface brightness, which gradually decreases towards the outer regions.
