The galaxy presents as a moderately luminous, elliptical structure. Its morphology appears largely smooth and undisturbed, with a high degree of central concentration. The light profile suggests a centrally dominant population of older stars, exhibiting a yellowish-orange hue. The galaxy's shape is elongated, but not to a significant extent; it appears moderately flattened. There is no discernible dust lane or spiral arm structure visible, indicating a lack of active star formation within the disk. No major merging features are apparent. There is only the slightest hint of tidal distortions, suggesting a possibility of recent interactions.
