The galaxy presents an overall elliptical morphology, though with some visible disturbances indicating potential interaction or recent merger activity. The central region exhibits a concentrated, bright yellowish core, suggesting a significant population of older stars. Fainter, bluish-green extensions are visible on either side of the core, hinting at possible tidal features or ongoing star formation in the outer regions. The galaxy appears relatively smooth in structure, with no distinct spiral arms readily apparent. The overall color profile suggests a moderate redshift, placing the galaxy at a considerable cosmological distance.
