The galaxy presents as a relatively smooth, elliptical structure with a concentrated, luminous core. Its overall color profile suggests an older stellar population, appearing more yellow and red-toned than blue. There is a slight elongation in its form, but it is largely roundish. No distinct spiral arm structures or prominent dust lanes are observed, although there are some very minor disturbances. Based on its appearance, it does not appear to be actively undergoing a major merging event.
