The galaxy presents an overall elliptical morphology, with a dominant smooth component. The light profile suggests a relatively evolved stellar population, exhibiting a redder color index. There appears to be a slight asymmetry or minor perturbation visible, potentially indicative of a past or ongoing minor merger event. The overall color suggests moderate levels of star formation. The approximate size indicates the galaxy is a moderately large, with an estimated stellar mass on the order of 10^11 solar masses.
