The galaxy presents as a flattened elliptical morphology, with a high degree of smoothness. The primary color is yellowish-orange, indicative of an older stellar population. There is a subtle color gradient, with the central region appearing more yellow. The axial ratio suggests a classification approaching E5 or E6 on the Hubble sequence. No obvious dust lanes or spiral arm structures are discernible, implying a lack of significant ongoing star formation. The general appearance suggests a relaxed system, unperturbed by recent major mergers, although minor disturbances cannot be ruled out based on this image alone.
