The galaxy presents as a generally smooth object, with a subtle disk-like structure. It appears to be elliptical in shape with a moderate degree of roundness. A bright central bulge is evident, with a slight color gradient outwards towards the edges of the galaxy. There is a hint of a minor disturbance or possible interaction on one side of the galaxy, perhaps suggesting ongoing or past merger activity. The light from this galaxy indicates that it is a relatively massive galaxy with a moderate rate of star formation.