This galaxy appears to be composed of two distinct components. The larger component has a diffuse, elongated morphology, suggesting a flattened spheroidal or possibly an edge-on disk structure. It exhibits a bluish hue, hinting at the presence of a younger stellar population and ongoing, albeit potentially low, levels of star formation. The smaller component is more compact and displays a yellowish coloration. This color suggests an older stellar population, implying a cessation, or significant reduction, in star formation activity within this region. There is a hint of tidal disturbance in the overall structure. The galaxy appears relatively smooth, but there is a potential distortion or minor interaction.
