This galaxy exhibits a relatively smooth morphology with an overall elliptical shape. The central region displays a concentrated, yellowish-white hue, suggestive of an older stellar population likely consisting of Population II stars. This contrasts with the outer regions, which appear bluer and more diffuse, hinting at the presence of younger stars and possible ongoing star formation. There are some indications of tidal disturbances or minor interactions, potentially with a smaller satellite galaxy, as evidenced by the slight asymmetry observed in the outer halo. These features are not pronounced, indicating a less energetic merging process. The galaxy appears to have an estimated stellar mass that is well within that of a typical galaxy. Overall, the galaxy presents as a somewhat evolved system with both old and relatively young stellar populations and possible recent or ongoing interactions that have slightly perturbed the established structure.
