The galaxy presents as a fairly regular, elliptical morphology with a smooth appearance. It appears to be relatively round, with a slight deviation towards an intermediate shape. There may be some minor disturbances present, but no major merging activity is visibly apparent. The color profile suggests a slightly redder population of stars, indicating an older stellar population or the presence of dust, and it is likely a massive galaxy. Star formation appears to be present, but at a lower rate.
