The galaxy presents a predominantly smooth morphology, suggesting an elliptical type. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness outward. There is a slight elongation, but no distinct spiral arms or bar features are visible. Faint hints of a disk may be present, but they are poorly defined. The color is generally consistent, with a slight redder hue in the central region which might be a sign of older stellar population or dust extinction. There is some evidence of a minor disturbance event, but it is not obvious.
