The galaxy presents an overall elliptical morphology, appearing moderately elongated rather than perfectly spherical. Its central region exhibits a concentrated, smooth luminosity, with a color profile shifting towards redder wavelengths. The outer regions display a bluer hue, although the overall color gradient suggests a relatively evolved stellar population. There's a subtle indication of a disk-like component within the galaxy; however, the lack of defined spiral arms or strong features indicates a mostly smooth stellar distribution. Some minor disturbances are evident, but major merger activity is not apparent. Star formation rate is expected to be low. Overall, the galaxy appears to be an intermediate system with evolving features.
