The galaxy appears to be a relatively smooth, elliptical galaxy. The central bulge exhibits a yellowish-orange hue, suggestive of an older stellar population dominated by red giant stars. Surrounding the core, there is a less concentrated and fainter blueish halo. The smoothness of the overall light distribution indicates a lack of significant dust lanes or spiral arm structures. There are possible minor disturbances present. Based on the morphology, this galaxy is unlikely to be undergoing a major merger event. The overall shape appears relatively round.
