The galaxy presents as a disk-shaped object, although precise classification is hindered by resolution limitations. The morphology is predominantly smooth with some features, showing a higher concentration of light towards the center. The primary component of light emitted by the galaxy appears to be shifted toward the redder end of the spectrum. There is an observable change in color moving from the center to the outer regions of the galaxy. At least a mild disturbance is present in the structure of the disk.
