The galaxy presents a largely smooth morphology. It appears relatively round in shape, with a high degree of central concentration as suggested by the color gradient moving out from a bright center. The color is weighted towards red. There is little evidence of prominent spiral arms or dust lanes, and it does not appear to be undergoing any major merging activity. There is some possibility of subtle internal structure suggesting some features like the hint of a disk, but these are minimal. The colors imply that the older stellar populations dominate the light output of the galaxy. The galaxy appears to be relatively undisturbed and quiescent.
