The galaxy appears to be a somewhat diffuse object, exhibiting a predominantly smooth morphology. There is a relatively bright, concentrated core. The light distribution transitions from blueish-white at the center to more greenish towards the edges. The outer regions show slight irregularities and hints of possible tidal disturbance or interaction with a smaller companion galaxy. Overall, the light appears somewhat homogenous, with no strong evidence of distinct spiral arms or a well-defined disk.
