The galaxy appears to be a relatively smooth, centrally concentrated system. The core exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions show a gradual decline in surface brightness, fading into a bluish halo. There is minimal evidence of spiral arm structure or prominent dust lanes. The overall shape is elongated, with the ratio of major to minor axes suggesting it is likely an elliptical galaxy. There are some irregularities in the outer regions that could potentially suggest minor disturbances or interactions. The lack of significant morphological features suggests a galaxy that has largely completed its major mergers. This is a fairly massive galaxy, which is also supported by it's low rate of star formation.
