The galaxy presents a primarily smooth, elliptical morphology. Its color profile exhibits a redder hue in the central region, suggestive of an older stellar population and/or dust obscuration, while the outer regions appear slightly bluer, indicating the presence of younger stars. The object is observed to have a high degree of roundness. There are subtle indications of minor disturbances in its structure that may point toward an ongoing or recent interaction/merger. However, no major asymmetries or tidal features are observed. Given the overall mass, it likely has a suppressed star formation rate.
