The galaxy presents as a somewhat smooth, ellipsoidal structure, though with some subtle irregularities. It is centrally concentrated with a bright core region that gradually fades outwards to its periphery. There are suggestions of a very faint, broad disk, though no distinct spiral arms are evident. There is a hint of what appears to be a disturbance in the galaxy's morphology. The color gradient appears to be consistent with an aging stellar population and ongoing star formation.
