The galaxy presents as a dual-component system with a notable interaction. The primary component exhibits a smooth, elliptical morphology with a yellowish hue, suggestive of an older stellar population and minimal ongoing star formation. The secondary component, positioned closely to the primary, appears less defined. It shows an irregular shape with a bluish tint, indicating the presence of younger, hotter stars and ongoing star formation. There is a slight bridge of light that could be tidal interactions.
