The galaxy appears to be a relatively smooth, elliptical system. Its light is concentrated towards the center, with a gradual decrease in surface brightness moving outwards. The overall color is slightly bluish-white, suggesting a moderate population of younger, hotter stars. There is no evidence of significant spiral arm structure or a prominent dust lane. The galaxy exhibits a generally round shape with a slight elongation, not appearing as a perfect sphere. There are no clear signs of any recent major merger events, although there could be some subtle disturbances present in the outer regions. Overall, the galaxy presents as a typical elliptical galaxy with a moderate amount of ongoing or recent star formation.
