The galaxy presents a largely smooth morphology, indicative of an elliptical or lenticular type. It exhibits a high degree of central concentration with a relatively symmetrical structure. There is a slight deviation from perfect circularity, leaning more towards a rounded shape. No distinct spiral arms or bar-like structures are visible. There is no major evidence of recent or ongoing mergers or interactions with other galaxies, although minor disturbances cannot be entirely ruled out. The color profile shows a reddish hue suggesting an older stellar population, implying low star formation activity.
