The galaxy presents a primarily smooth morphology, with a high concentration of light towards the center. It is elliptical in shape, though only slightly elongated. The central region exhibits a yellowish hue, suggestive of an older stellar population. The outer regions fade in intensity, displaying a bluer color, potentially indicating younger stars. There appears to be no prominent spiral arm structure or significant dust lanes visible. The overall impression is that of a relatively undisturbed galaxy, with no obvious signs of a major ongoing merger, or a major disturbance. The galaxy shows no particular signs of being a disk galaxy.
