The galaxy presents as an elongated, ellipsoidal structure. It exhibits a smooth, relatively featureless morphology, lacking prominent spiral arms or a distinct bar. The central region displays a concentration of light, appearing brighter and more yellow in color. This may be due to a large concentration of older stars, as well as dust extinction of blue light. The outer regions of the galaxy are less defined, with a gradual decrease in surface brightness moving outwards. The light profile exhibits a Sersic index value suggesting a morphology between a pure exponential disc galaxy and an elliptical galaxy. The color gradient suggests a possible difference in stellar populations between the bulge and disk components.
