The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a concentrated central bulge that graduates outward into a more diffuse halo. The central region is characterized by a yellowish-orange hue, suggestive of an older stellar population with relatively low levels of on-going star formation and a possible accumulation of dust. The lack of distinct spiral arms or other clear morphological features such as bars or rings supports its classification as an elliptical galaxy. There is some slight disturbance in the halo, possibly caused by a minor merger.

