The galaxy appears to be an elliptical type, exhibiting a smooth, largely featureless morphology. It presents with a bright central bulge, suggesting a concentration of older stellar populations. The light profile is somewhat elongated but generally rounded, transitioning gradually from the bright core to the fainter outer regions. There appears to be possible tidal disturbances with an arm-like structure that is seen on the left. Evidence indicates that this galaxy may be in the process of merging.
