The galaxy presents as a generally smooth, somewhat rounded structure. There is a slight ellipticity apparent, but it appears mostly circular. The core is bright, with the luminosity decreasing gradually outwards. The galaxy exhibits a color gradient, transitioning from bluer hues in the central region to redder tones in the outer regions. The overall color suggests a moderate age stellar population, possibly with ongoing, albeit subdued, star formation in the core. There is no clear evidence of spiral arm structure or a prominent disk. There are no obvious signs of a major merger event, although a slight asymmetry in the outer regions might indicate minor past interactions. The smoothness of the galaxy suggests it may be an early-type galaxy or a lenticular galaxy seen face-on.
