The galaxy presents a largely smooth, elliptical morphology. The core exhibits a high degree of central concentration, with a bright, relatively uniform yellow-orange hue, indicative of an older stellar population. There is a subtle radial falloff in luminosity from the core outwards. There is no visible evidence of spiral arm structure or significant dust lanes. The outer regions appear very smooth and diffuse, lacking any distinct features indicative of active star formation. No signs of tidal tails or distortions suggest any recent major merger events. There appears to be slight red shift, indicative of a high degree of separation from our own galaxy.
