The galaxy presents as a relatively compact structure with a smooth, elliptical morphology. It exhibits a moderate level of central concentration, with a gradual decrease in surface brightness outwards. There is a subtle elongation visible, suggesting a deviation from perfect sphericity. No distinct spiral arms or bar structures are apparent. The overall color appears consistent with an older stellar population, showing a bias toward redder wavelengths. No significant dust lanes or prominent star-forming regions are observed. Faint wisps or tidal features may be present in the immediate vicinity, potentially indicating past or ongoing minor interactions with smaller satellite galaxies, though this is not entirely conclusive based on the available image.
