The galaxy exhibits a disturbed morphology, possibly indicative of a past or ongoing interaction. The central region is dominated by a smooth, bright component appearing almost spheroidal in shape. Two distinct features are visible on either side of this central region. They are less prominent than the central region and show a yellowish-orange hue. These could be tidal tails, remnants of a spiral structure, or clumps of star formation. The system appears relatively isolated. The dominant color of the core is bluer when compared to the outer regions. Given the morphology, the galaxy may have an elevated star formation rate. The overall size is compact.
