The galaxy presents as a lenticular or possibly early-type spiral morphology, viewed at a significant inclination. A prominent bulge dominates the galactic structure, exhibiting a smooth, centrally concentrated luminosity profile, yellowish colouration suggesting an older stellar population. The disk component, though present, is not clearly resolved into spiral arms, potentially due to the viewing angle or a lack of prominent star formation. It shows a bluer colouration on one side suggesting a younger stellar population. Faint disk-like structure extends outwards. Overall, the galaxy appears to be relatively undisturbed, exhibiting no obvious signs of major merger activity. A faint companion galaxy is visible.
