The galaxy appears to be a disk galaxy, although it is not viewed face-on. It is seen at an oblique angle, allowing for some estimations of its shape. It shows a distinct central bulge that appears relatively smooth and concentrated. The disk component exhibits a degree of asymmetry. The overall color of the galaxy appears to be on the redder side, suggesting an older stellar population and/or significant dust obscuration. There are hints of spiral arm structures within the disk, though they are not clearly defined. The galaxy is elongated. There is minor evidence of tidal disruption, such as a faint stream, but is not a significant feature.
