The galaxy presents a generally elliptical morphology, appearing relatively smooth and undisturbed. Its central region exhibits a concentrated, bright luminosity, suggesting a high stellar density. Moving outward from the core, the luminosity decreases gradually. The central area displays a yellowish hue, potentially indicating an older stellar population. Faint extensions emanate from the central region, displaying a greenish tinge. The galaxy exhibits an intermediate roundness. There is no evidence of substantial tidal interactions or mergers.
