The galaxy presents as a concentrated object with a smooth morphology, displaying a distinct lack of spiral arms or other prominent features typical of disk galaxies. The central region exhibits a significantly higher surface brightness, appearing almost spheroidal. Evident is a pronounced color gradient; the core displays a yellowish-orange hue, suggesting an older stellar population and reduced star formation activity. The outer regions fade into a bluish-white halo, potentially indicative of a younger, bluer stellar population, although this is far less prominent. There is what appears to be an object near the galaxy that appears to be interacting with it. It looks like this object is either in the middle of merging with the galaxy or is in the process of being pulled apart due to tidal forces.
