The galaxy exhibits a generally smooth, elongated morphology, with a high degree of axial ratio suggesting an elliptical shape. The central region displays a concentration of light with a yellowish hue, possibly indicating an older stellar population. The outer regions show hints of a disk, with a bluer color indicative of ongoing star formation. There are also some signs of minor disturbances. Overall, the galaxy seems to be a transitional object, perhaps evolving from a spiral to an elliptical shape.
