The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears fairly uniform, lacking prominent spiral arms or distinct features. There is a slight elongation, suggesting it is not perfectly spherical. The color is predominantly a yellowish-white hue, indicative of an older stellar population. No significant dust lanes or active star-forming regions are apparent upon visual inspection. There may be a very slight disturbance in its structure, but it is faint. The galaxy appears to be largely isolated, showing no signs of a major merger in progress.
