The galaxy presents as a relatively smooth object, with a diffuse, centrally concentrated light profile. The dominant color is a reddish-yellow hue, suggesting an older stellar population and a low rate of on-going star formation. There is a slight elongation of the galaxy along its major axis, but it largely appears to be of an elliptical form rather than a spiral. No distinct spiral arms or prominent dust lanes are discernible. There are some indications of possible tidal disturbances with faint, diffused light, implying this galaxy may have merged with another galaxy. 