The galaxy presents an overall elliptical morphology, appearing largely smooth and relatively compact. Evident within the galaxy are two distinct regions. One region displays a yellowish-orange hue, suggesting an older stellar population or significant dust extinction. Adjacent to this is a bluer, whiter region, which likely indicates a population of younger, hotter stars, and ongoing or recent star formation. Given the proximity and irregular shapes of these two color regions, this could be a system experiencing a merger event, or a galaxy with a disturbed morphology. Faint tidal tails or streams are not clearly discernible, though this could be due to limitations of image resolution. The galaxy's concentration appears intermediate, neither highly centrally concentrated nor completely diffuse.
