The galaxy presents as a single, relatively smooth, and centrally concentrated object. Its shape is broadly elliptical, appearing mostly round, with a slight tendency towards elongation. A dominant central bulge is evident, emitting strongly in the yellow-red wavelengths. The light profile diminishes steadily from the core, suggesting a fairly uniform stellar population density throughout the visible extent of the galaxy. There is no indication of prominent spiral arms, bars, or dust lanes. The galaxy displays a fairly homogenous color profile with a yellow hue throughout, suggesting the presence of an older stellar population and little active star formation. There is no visible evidence of any major ongoing merger events. The lack of blue light indicates a quiescent system with minimal recent star formation.
