The galaxy presents a morphology suggestive of a recent or ongoing interaction. The overall shape is irregular, deviating significantly from a simple elliptical or spiral form. Two distinct components are visible: A brighter, centrally concentrated region exhibiting a bluish hue, and a more diffuse, elongated structure with a yellowish-orange color gradient. The brighter region might indicate a concentrated area of star formation, which could explain its blue appearance. The elongated structure appears disrupted with indications of tidal tails. This may be the result of gravitational interactions between the galaxy with another object. The color gradient in the elongated structure indicates varying stellar populations, with older populations dominating the yellowish-orange regions. Given its appearance, the galaxy appears to be undergoing a merger.
