The galaxy presents as a centrally concentrated, elliptical structure. The light distribution appears smooth with a high degree of central concentration. There is little evidence of spiral arm structure, dust lanes, or other distinct morphological features, instead a fuzzy and diffuse disk-like morphology is detected. The color profile suggests an older stellar population, as indicated by the reddish-yellow hue, with only trace amounts of star formation occurring within the galaxy. It shows no apparent signs of major mergers or significant tidal disturbances in its immediate environment. It has a generally round shape with a major to minor axis ratio near 1:1.
