The galaxy presents as a disturbed system, likely undergoing a merger. There are two distinct components, one with a bluish-white hue, and a second, more diffuse component with a yellowish-orange color. The bluish-white component appears relatively smooth with no visible substructure. In comparison, the yellowish-orange component exhibits a significantly less symmetric distribution of light, with a noticeable elongation and what appears to be disturbed morphology and tidal features. The estimated size is approximately 6.7 kpc across. Its morphology suggests a relatively high degree of central concentration. It shows signs of moderate star formation activity. The overall appearance strongly indicates a galaxy interaction or merger event.
