The galaxy appears as a single, centrally concentrated object. It exhibits a generally smooth and rounded morphology, with no obvious spiral arms or significant disk structure discernible in the image. The light profile suggests a high degree of central concentration, with luminosity decreasing smoothly from the core outward. The color profile is subtle, exhibiting a yellowish core with a slight transition to greener outer regions, suggesting older stellar populations dominating the central region, with hints of ongoing star formation in the outskirts. No major merging signatures are present, indicating a relatively undisturbed system. Minor disturbances may be subtle or undetectable at this image scale.
