The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a concentrated, bright yellowish-white luminosity, which gradually diffuses outwards into a less defined halo. The outer regions appear fainter and display a slightly bluer hue, suggestive of differing stellar populations or ongoing star formation, although the galaxy lacks any obvious spiral arm structure. A high degree of radial symmetry is apparent. There is no evidence of significant tidal disturbances or ongoing mergers. The galaxy appears to be a well-formed, relatively quiescent system.
