The galaxy exhibits a complex morphology with both smooth and featured characteristics. A dominant, relatively bright central bulge or core region is visible, appearing somewhat amorphous, with a slightly elliptical shape. There is indication of disk-like structure surrounding this central region. Definite features indicate a perturbed or disturbed state, suggesting a recent or ongoing interaction with another galaxy. One tidal tail or streamer of material extends outwards in a non-symmetric direction, reinforcing the idea of gravitational disturbance. The galaxy does not appear to be a simple elliptical nor a clear spiral but has a combination of both types of features along with clear signs of a recent interaction.
