The galaxy presents as a somewhat elliptical, disk-like structure. The central region exhibits a high degree of luminosity, suggesting a concentrated nucleus likely harboring a supermassive black hole. Proceeding outward from the nucleus, the intensity of the light gradually decreases. There is subtle evidence of spiral arm structures, though they appear somewhat disrupted or flocculent. Patches of redder light are seen, possibly indicative of regions of ongoing or recent star formation activity within gas and dust clouds. The overall color profile suggests a population of intermediate to old stars, contributing to the yellow hue of the galaxy. There is no major merger activity apparent in this image, though a minor disturbance cannot be ruled out. The galaxy appears to be fairly well-defined, with a relatively smooth profile. 
