The galaxy appears to be primarily smooth in morphology, exhibiting a concentrated central bulge. There may be a faint disk-like structure to one side of the galaxy, though this could be an artifact of observation or a minor irregularity in the galaxy's shape. The overall shape seems fairly round. Evidence suggests it is not undergoing a major merger, but a minor interaction or disturbance cannot be ruled out. The galaxy exhibits a strong emission signature in the green wavelengths. The relatively high intensity and concentrated light profile suggest a likely early-type classification or a late-type with a significant bulge component.
