The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, appearing significantly elongated rather than circular. A discernible color gradient is observed, transitioning from a yellowish, luminous core to a bluer, more diffuse outer region. The galaxy lacks any apparent spiral arm structure or distinct features suggesting active star formation. There are subtle hints of tidal disturbances present, likely indicating minor interactions or mergers. The surrounding halo is faint and poorly defined, fading gradually into the background sky. Overall, the galaxy appears as a mature system, likely dominated by an older stellar population.
