The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness and rotational symmetry. The luminous core region transitions gradually into the outer halo without any discernible substructure. The galaxy color suggests it is comprised primarily of older stellar populations. There is no clear evidence of spiral arms or active star formation regions visible. The lack of irregular features suggests a quiescent state, undisturbed by any recent major merger events. The galaxy appears to be a relatively isolated system within its local environment.
