The galaxy presents a predominantly smooth morphology, with an elliptical appearance. The light distribution suggests it is moderately centrally concentrated. Its overall shape is more closely described as being between round and elliptical. There is weak visual evidence of a disk. There is some structural disturbance visible, possibly hinting at a minor interaction or past merger event, but this is relatively subtle. The galaxy exhibits a reddish hue, with the light having a median g-band absolute magnitude in the -19's, median r-band absolute magnitude in the -20's, and a median z-band absolute magnitude in the -21's. Based on inferred star formation rates (SFR), star formation activity is quiescent. It should be noted that the inferred stellar mass is roughly 10^10 solar masses.
