The galaxy presents as a disk galaxy with an elliptical morphology, appearing moderately smooth in overall texture. It exhibits a prominent, bright central bulge that is yellow-orange in color, suggesting an older stellar population. The disk is visible, and its bluer hue indicates the presence of younger stars and ongoing star formation. The disk shows faint signs of structure, possibly weak spiral arms or irregular dust lanes, though these are not sharply defined. There might be signs of a minor disturbance in the disk morphology, indicating possible past interactions. There is no clear evidence of a major merger event. The galaxy's intermediate axial ratio suggests it is being viewed at a significant inclination angle.
