The galaxy presents as a centrally concentrated, primarily smooth object. The light distribution suggests a spheroid-dominated morphology. Its overall shape is elliptical, approaching round, with a very slight elongation evident. There is a color gradient, with the central region appearing more yellow-white, suggesting an older stellar population, while the outer regions exhibit hints of redder hues. No prominent spiral arm structures or significant dust lanes are discernible. The overall appearance indicates a galaxy that is relatively quiescent in terms of ongoing star formation. There is no indication of any major mergers, although there are faint wisps suggesting minor disturbances.
