The observed galaxy presents as a relatively smooth, elliptical morphology. There is a concentrated central bulge that appears to be surrounded by a slightly fainter, more diffuse halo. The color profile suggests an older stellar population and a relatively low rate of current star formation within the visible region. The galaxy appears largely undisturbed, showing no signs of major mergers or significant tidal interactions. It is a generally round shape, showing an ellipticity close to zero. 
