The galaxy appears as a flattened, disk-shaped structure viewed edge-on. There is a prominent central bulge, exhibiting a smooth, concentrated light profile. The disk component shows some subtle variations in surface brightness, hinting at possible spiral arm structures but these features are indistinct. The overall color of the galaxy is moderately blue, especially in the outer disk regions. This suggests the presence of ongoing star formation, with younger, hotter stars contributing to the blue light. There are no obvious signs of significant tidal disturbances or interactions with other galaxies. The galaxy presents as a relatively isolated, mature system.
