The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light distribution. There is no evidence of spiral arms or a prominent disk structure. The color appears generally yellow to orange, suggesting a stellar population dominated by older, redder stars. The isophotes are generally elliptical, appearing mostly round, with only slight elongation. There are no obvious signs of ongoing major mergers or tidal disturbances. The galaxy exhibits a relatively compact structure. The color suggests a relatively low star formation rate.
