The galaxy presents as a disturbed system, likely undergoing a merger event. There appears to be two primary components, with the larger of the two exhibiting an elongated morphology. This primary body shows some hints of disk-like structure, but it is heavily disrupted. It also appears to be relatively smooth in texture with a yellowish hue. The secondary component shows a more spherical shape. There is no spiral structure visible, and there are significant tidal features. The tidal features are elongated and seem to reach out from the merging galaxies. The color distribution of the galaxy suggests a fairly old stellar population with limited ongoing star formation.
