The galaxy presents a primarily smooth, elliptical morphology. The core region is characterized by a high surface brightness, appearing nearly unresolved and intensely luminous. Moving outward, the light gradually diffuses into a halo with a somewhat irregular shape. Hints of faint, elongated tidal features suggest the possibility of past or ongoing minor interactions with another galaxy. The light distribution appears slightly bluer in the central region and shifts towards redder tones further out. No distinct spiral arms or dust lanes are visible.
