This galaxy exhibits a somewhat regular, though not perfectly elliptical, morphology. It presents a distinct color gradient, appearing brighter and more yellow-white towards its central region, suggesting a higher concentration of older stellar populations in the core. Surrounding this core is a region with a distinct blue-violet hue, possibly indicating active star formation or a population of younger, hotter stars. The distribution of light appears relatively smooth across the galaxy, although there might be hints of some underlying structure within the outer regions. Overall, the galaxy's light distribution suggests a relatively mature system that may have experienced some recent star formation activity. There is an indication of a possible minor disturbance in the disk.
