The galaxy presents a predominantly smooth morphology, characterized by a centrally concentrated bulge. There is little to no visible disk structure. The galaxy appears relatively round, exhibiting a moderate degree of ellipticity. Its color is primarily yellowish-orange, indicative of an older stellar population. There is no obvious evidence of a recent major merger event, although slight asymmetry in the outer regions could suggest a minor interaction or disturbance. The overall structure suggests an evolved system with a relatively low rate of current star formation.
