The galaxy presents as a single, centrally concentrated object. It is generally elliptical in shape. Its core exhibits a bright, yellowish hue, suggesting an older stellar population. The outer regions appear more diffuse and show hints of a bluer tint, although this is quite subtle and might be due to younger stars or ongoing, albeit low, star formation. There is no evidence of spiral arms or a distinct disk structure; the galaxy appears relatively smooth. There are no signs of any major ongoing mergers or significant tidal disturbances visible in the image. Overall, the galaxy seems to be a relatively evolved system.
