The galaxy presents as a centrally concentrated system with a smooth, rounded morphology. A bright, relatively compact core is visible, transitioning into a fainter, more diffuse halo. The color profile appears to be relatively uniform across the galaxy, showing a subtle bluer hue in the outer regions. There is no apparent spiral structure or distinct features, such as dust lanes or prominent star-forming regions, observable in this image. The overall appearance suggests a relatively evolved system with a low ongoing star formation rate. The size is consistent with a typical galaxy at its redshift. There is no obvious evidence of any major interactions or merging events.
