The galaxy presents a smooth, relatively featureless appearance. It is roughly elliptical in shape, exhibiting a high degree of central concentration of light. The color gradient suggests a redder core with bluer outer regions, potentially indicative of an older stellar population in the center and younger stars towards the periphery. There is no readily apparent spiral structure or bar. Minor disturbances appear to be present. Overall the galaxy appears fairly isolated. The estimated size, based on light distribution, appears to be a modest few kiloparsecs in radius.
