The galaxy appears as a fairly smooth, centrally concentrated object with a generally elliptical morphology. There is some indication of a slight disk, but the dominant impression is that of a bulge component. The color profile suggests an older stellar population, appearing more yellow/red, consistent with reduced star formation. There is no evidence of active galactic nuclei, strong dust lanes, or obvious tidal disturbances suggesting a recent merger event or strong interaction with another galaxy. The overall impression is that of a relatively undisturbed galaxy with a substantial spheroidal component and subdued star formation.
