The galaxy presents an overall elliptical morphology, appearing relatively smooth and possessing a somewhat elongated shape. Its central region exhibits a high surface brightness, indicative of a concentrated stellar population, while the outer regions gradually fade into the background sky. The light distribution suggests a centrally concentrated structure without pronounced spiral arms or distinct features, aside from a slight elongation. A subtle color gradient can be observed, where the central regions appear more yellow-white, suggesting an older stellar population, in contrast to a somewhat bluer hue in the outer regions that potentially indicates more recent star formation. There is no evidence of significant dust lanes or prominent star-forming regions. Overall, the galaxy appears as a fairly undisturbed, evolved system.
