The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy, viewed at an oblique angle. It displays a prominent, bright central bulge that seems to dominate the galaxy's overall luminosity. There is little evidence of active star formation in the image, with no discernible blue knots or HII regions.

The disk is subtly visible, exhibiting a somewhat elongated shape. Dust lanes are not clearly apparent, suggesting the galaxy is relatively evolved and gas-poor. The outer regions of the disk fade gradually, indicative of a smooth transition in stellar density. There are no signs of any major ongoing merger events. The slight asymmetry on the edges could indicate minor tidal disturbances or interactions.
