The galaxy presents a smooth, elliptical morphology. Its light profile appears centrally concentrated, exhibiting a bright, yellowish core that gradually fades into a less defined outer halo. There is no discernible spiral structure or prominent dust lanes. The overall color suggests a population dominated by older stars, which, when considered alongside the smooth morphology, supports a classification as an elliptical galaxy. Its shape appears largely spherical, with no evidence of significant tidal disturbances or ongoing merger activity. Based on the absence of obvious features associated with active star formation, star formation is expected to be low. 
