The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color is on the redder end of the spectrum, with a concentrated, bright central bulge. The outer regions of the galaxy fade smoothly into the background, showing little evidence of distinct spiral arms or irregular features. There may be very slight elongation present. No strong signs of recent or ongoing major mergers or tidal disturbances are immediately apparent. The overall morphology suggests a relatively evolved system dominated by an older stellar population with a low star formation rate.
