The galaxy presents as a diffuse object with a moderate angular size. It exhibits a somewhat amorphous morphology, lacking a clearly defined spiral or elliptical structure.

There is a hint of a disk-like component. However, this structure appears disrupted, possibly due to gravitational interaction with another galaxy. A notable feature is a prominent central bulge which appears rather smooth.

Color gradients suggest varying stellar populations and dust distribution within the galaxy. The central bulge exhibits a slightly redder hue, possibly indicating an older stellar population. Distortions are evident, suggesting a possible recent or ongoing merger event. Faint tidal features or tails may be present.
