The galaxy presents a largely smooth, elliptical morphology. It exhibits a radial profile that steadily decreases in intensity from the center outwards, with a high degree of central concentration. There is no obvious spiral arm structure or significant disk component discernible in this observation. The galaxy appears nearly circular, showing minimal signs of elongation or asymmetry. No prominent tidal features or merging signatures are immediately apparent; the overall structure suggests a dynamically relaxed system. The galaxy appears to be undergoing relatively low levels of star formation, as suggested by the subtle color gradients across its body. The core region emits strongly, suggesting an active region in the nucleus.
