The galaxy appears as a moderately sized object with an approximate elliptical shape. It exhibits a diffuse, luminous halo surrounding a more compact central region. The central region shows some evidence of structure, but appears to be a combination of disk and irregular features. It may be a galaxy undergoing a merger or some sort of tidal stripping. The outer halo is not smooth.

The color distribution indicates variation within the galaxy. The central regions display bluer colors, potentially indicating younger stellar populations or active star formation. Some regions are more red, indicating areas of older stars.

The overall morphology suggest an elliptical galaxy with unusual features, or some sort of disk galaxy undergoing a merger or disturbance.
