The galaxy appears as a lenticular or early-type spiral, exhibiting a moderately flattened, disk-like structure. A central bulge is discernible, showing a brighter, more concentrated luminosity profile compared to the outer regions. The galaxy appears mostly smooth with a subtle disk-like structure, and a slight cigar shape. There is no distinct spiral arm structure visible, suggesting that it may have either very tightly wound arms or none at all. There may be some indication of minor tidal disturbances, but it appears generally isolated with no major ongoing mergers. The color profile is relatively homogenous across the galactic body.
