The galaxy presents as a relatively smooth, elliptical or lenticular type, exhibiting a centrally concentrated light profile. There is a distinct lack of spiral arm structure. The color indices suggest a population of older stars; a reddish hue is visible in some areas.  The galaxy appears to be experiencing a low rate of star formation. There is a potential hint of a minor tidal interaction or disturbance in its upper regions. The galaxy’s morphology is classified as intermediate between rounded and elongated. No major merger activity is obvious, though minor disturbances are present.
