The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual falloff in surface brightness towards the outer regions. The core of the galaxy exhibits a yellowish hue, possibly indicating an older stellar population. The overall shape is generally round. There are no readily apparent spiral arms or strong dust lanes. There is a small amount of blueish hue within the object, possibly indicting a younger stellar population. There appears to be no major ongoing merger activity or tidal disturbances are visibly interacting with the galaxy.
