The galaxy presents as a relatively smooth object, generally elliptical in appearance. The main body exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity towards the outer edges. There is a hint of tidal disturbance with a distinct secondary body close to the main galaxy, suggesting a potential ongoing or recent interaction or minor merger event. There are very faint traces of diffuse light potentially indicating tidal streams or disrupted morphology. The central region is dominated by bluer wavelengths, potentially indicative of a population of younger, hotter stars. The extended halo surrounding the galaxy exhibits redder colors. This suggests a potentially older stellar population. The shape shows slight deviations from a perfect circle, showing it may be slightly elongated.
