The galaxy presents an overall disturbed morphology. A relatively bright, somewhat rounded central region is apparent, exhibiting a bluish-white hue, potentially indicative of a population of younger, hotter stars. Emanating from this central region is a distinct feature appearing as a tail or stream, also bluish in color, suggesting an ongoing or recent interaction or merger. The galaxy displays a moderate level of star formation. The object is relatively small, but not compact. The general appearance is somewhat distorted and hints at tidal features. Overall, the galaxy's structure suggests an active stage, possibly influenced by external gravitational forces.
