The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright yellowish-white core, indicative of an older stellar population. The galaxy appears relatively round. Fainter, diffuse bluish light surrounds the central core, possibly suggesting some low-level star formation activity within a disk-like structure. No signs of significant tidal disturbance or ongoing major merger events are immediately apparent. The overall structure indicates a galaxy that is either an elliptical galaxy or a spiral galaxy with a prominent bulge and a disk that is viewed nearly face-on. 
