The galaxy appears to be a single, relatively smooth structure, with a high degree of central concentration. The overall shape is elliptical, appearing quite round. There is a suggestion of some tidal disturbance, which is likely the result of a minor merger or interaction with a companion galaxy. There is a slight asymmetry in the galaxy's outer regions.

The color distribution suggests a population of older stars, giving it a reddish or yellow hue. Star formation is present, although likely not at a high rate, resulting in slightly bluer regions that are visible.
