The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The light distribution is fairly symmetrical. There is a slight elongation and a lack of distinct spiral arm structures. It appears yellowish-white in color, suggestive of an older stellar population with fewer young, massive stars. No clear dust lanes or regions of active star formation are visible. There is no evidence of any major merger events, only a slight disturbance. The galaxy appears fairly undisturbed and relaxed.
