The galaxy presents an overall elliptical morphology when observing the shape of the isophotes. It appears to be a disk galaxy, seen at a moderate inclination angle. A bulge is visible that dominates the central region of the galaxy, with an orange hue, likely indicating an older stellar population. The galaxy's disk displays spiral arm structures, but they are not well-defined; instead, they appear somewhat flocculent. Patches of bluer light, indicating the presence of star formation, are also evident. There is no clear sign of major mergers or tidal disturbances from interactions. The galaxy appears to be relatively undisturbed in terms of its overall structure.
