The galaxy presents as a somewhat elongated, lenticular or early-type spiral morphology. The central bulge appears bright and relatively smooth, exhibiting a concentrated luminosity profile. A faint, diffuse disk component is discernible, but lacks significant spiral arm structure. Color gradients indicate a bluer color in the outer disk regions relative to the redder bulge, potentially suggesting ongoing, albeit low, star formation in the disk. The galaxy shows some evidence of minor tidal disturbance or asymmetry in the outer regions. The overall appearance suggests a galaxy that is in a relatively evolved state, with ongoing but subdued star formation activity.
