The galaxy presents as a lenticular, disk-shaped system, viewed at a significant angle to our line of sight. The central bulge is pronounced, exhibiting a bright, concentrated luminosity, possibly indicative of an older stellar population. The disk component is visible, though lacking distinct spiral arm structure. The color of the galaxy appears relatively uniform across its structure, trending towards redder wavelengths. There is some slight asymmetry in the shape of the disc which could point towards a past or ongoing interaction with another galaxy, however there is no distinct visual disturbance.
