The galaxy presents an elliptical morphology, exhibiting a generally smooth, featureless structure with a high degree of central concentration. Its color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue of the galactic core, possibly accompanied by intermediate star formation. The spheroidal shape indicates minimal rotational support and is consistent with a system dominated by random stellar orbits. There appears to be no evidence of significant tidal interactions or recent major mergers. The relative lack of internal substructure and the high degree of axial symmetry further support the classification as an elliptical galaxy in a relatively quiescent state, with a high degree of smoothness and homogeneity in its stellar distribution.
