The galaxy appears to be a relatively smooth, elliptical system. Its light is concentrated towards the center, exhibiting a gradual decrease in surface brightness with increasing radial distance. The core is a bright, yellow-white color indicating older stellar populations. There is no discernible spiral arm structure or dust lane obscuration. The shape of the galaxy appears largely spherical, with a minor elongation. There are no significant signs of tidal disturbances or ongoing mergers, although subtle asymmetries cannot be ruled out without higher resolution data. The overall color suggests a quiescent galaxy, with little active star formation.
