The galaxy exhibits a largely smooth morphology. A roughly circular, concentrated central region is apparent. The color distribution is not uniform, with a distinct color gradient observed, from a blue hue to a reddish hue at the center. There is no strong evidence of spiral arms or other disk-like structures, but there is some disturbance around the galaxy indicating the presence of dust. There seems to be little-to-no current star formation activity. It has a median radius of approximately 2.88 arcseconds. There does not seem to be another galaxy nearby with which it is merging.
