The galaxy presents as an interacting system, likely in the early stages of a merger. Two distinct galactic nuclei are visible, each surrounded by a diffuse halo of light. The larger of the two appears to be more spherical and displays a yellowish hue, suggesting an older stellar population. The second nucleus is less defined and possesses a bluish tint, potentially indicating more recent star formation activity. A faint bridge of material connects the two galaxies, implying gravitational interaction and tidal disruption. The overall shape of the system is irregular, deviating significantly from a standard elliptical or spiral morphology. The system shows signs of disturbance, further supporting the ongoing merger hypothesis.
