The galaxy presents a smooth, elliptical morphology. Its color profile suggests a higher concentration of older stellar populations, emitting primarily in the redder wavelengths. The overall structure indicates it is relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. There is a slight elongation in the shape and an absence of prominent spiral arms or distinct features that would indicate ongoing, large-scale star formation. The galaxy appears moderately luminous.
