The galaxy presents as a generally smooth, elliptical morphology. The light profile is centrally concentrated, with the brightest region being a somewhat diffuse core. The overall color is a yellowish-white, suggesting a relatively older stellar population with diminished recent star formation. A slight elongation is observed, deviating from a perfectly circular shape, but no distinct spiral arms or significant dust lanes are apparent. There is very little in the way of substructure visible; it seems to be a fairly uniform galaxy. There may be a very slight indication of tidal disturbances or interactions, though that is difficult to concretely determine based on available data.
