The galaxy presents as a centrally concentrated, relatively smooth object with a slight elongation. The core exhibits a yellowish-orange hue, which could indicate an older stellar population. A faint, disk-like structure with a bluer color component is observed surrounding the core. No distinct spiral arm structures or prominent dust lanes are readily apparent. There seems to be a slight disturbance in the morphology of the disk. The overall form of the galaxy appears relatively undisturbed.
