The galaxy presents a somewhat amorphous, disturbed morphology, likely indicative of an ongoing or recent interaction or merger event. The central region exhibits a brighter, more concentrated luminosity. There appears to be a dominant central concentration which may be a core, along with some extended structure. There is a hint of tidal tails. The color profile suggests a population of intermediate to old stars, with a possible pocket of star formation indicated by slightly bluer tones. The overall structure lacks well-defined spiral arms or a smooth elliptical shape, implying a dynamically active system. 
