The galaxy presents as an elliptical system with an apparent smooth morphology. The central region exhibits a higher surface brightness concentration, gradually decreasing towards the outer edges. The overall shape is approximately in between being round and elliptical. There are no prominent spiral arms or distinct features suggestive of strong ongoing star formation. Slight asymmetries or disturbances may indicate a minor interaction or past merger event. There does not appear to be a significant amount of dust obscuration within the galaxy. The colour appears to be dominated by bluer wavelengths.
