The galaxy presents as a centrally concentrated object with a generally smooth light distribution. There is little evidence of distinct spiral arm structures or significant dust lanes within the visible light. The color appears somewhat uniform across the galaxy, exhibiting a subtle yellowish-white hue. Given the absence of prominent features, the morphological classification is likely elliptical. The lack of blue color indicates that it is likely composed of older stellar populations, which might be relatively quiescent in terms of active star formation. It appears round in shape with no observable distortions.
