The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. A color gradient is observed, transitioning from a yellowish-orange core to a bluer, fainter halo. The galaxy does not exhibit any prominent spiral arms or distinct features suggestive of active star formation regions. The isophotes appear relatively regular, indicating a relaxed and dynamically evolved system. There is a slight asymmetry, possibly related to minor interactions or internal dynamics, but no major disturbances or merger events are readily apparent. Overall, the galaxy's appearance suggests an early-type morphology, consistent with an elliptical classification.
