The galaxy exhibits a disturbed morphology, indicative of a possible interaction or merger event. Its overall shape is elongated and irregular, deviating significantly from a pure elliptical or spiral form. There is an intense bright and concentrated central region, that appears yellowish. Extending away from this core is a region that is elongated. There is a very faint blueish color in this region, especially at the end. This area of lower surface brightness possibly contains younger stellar populations or dust lanes. There is a small orange clump that lies away from the main part of the galaxy. This might indicate a tidal tail or a dwarf galaxy companion undergoing accretion. Overall, this object appears to be a system in a state of flux, influenced by ongoing gravitational interactions.
