The galaxy presents as a relatively smooth, elliptical structure. It appears to have a concentrated central bulge which emits a yellowish light, suggesting an older stellar population. The overall shape approximates a circle, with only a very subtle elongation discernable. There are no visible spiral arms, bar structures, or other prominent features typically associated with younger, more active galaxies. Faint extensions of light can be observed. No indications of on-going major merger events are apparent.
