The galaxy presents as a single, relatively smooth object with a concentrated central bulge. There is little evidence of spiral arm structures or significant dust lanes. The morphology is generally elliptical or spheroidal in appearance, exhibiting a high degree of central concentration. The color gradient transitions from a yellowish-white core to a fainter bluish halo, suggesting a moderate population of younger stars residing outside of the core. Overall, it presents as a relatively undisturbed, mature system, with possible indication of recent, minor disturbances, such as star formation. 
