The galaxy presents as a centrally concentrated, largely smooth structure with a subtle elongation. The core exhibits a bright, yellowish hue indicative of an older stellar population and perhaps dust. The outer regions fade gradually into the background sky, with a hint of redder color indicating a possible presence of dust or a change in stellar population. There is no clear evidence of spiral arms or a well-defined disk structure. Overall, the morphology appears consistent with an elliptical or lenticular galaxy viewed from a significant distance, demonstrating an evolved state with low ongoing star formation. There is no obvious sign of merging or major disturbances.
