The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a generally smooth morphology. The central bulge is prominent, displaying a yellowish-white hue that suggests an older stellar population. The disk component appears relatively faint and flattened, with a subtle blueish tint along the edges, potentially indicating ongoing, but low-level, star formation activity. There is a slight asymmetry to the overall shape, but no obvious signs of major disturbances or ongoing mergers. The galaxy is elongated, leaning closer to a cigar shape, rather than being perfectly circular. 
