The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The light profile suggests a possible elliptical galaxy, given the lack of discernible spiral arm structure. A color gradient is observed, with the central region exhibiting a redder hue, possibly indicating an older stellar population. The outer regions appear bluer, suggesting the presence of some younger stars or star forming regions, although these are not pronounced. The galaxy appears relatively undisturbed, without any obvious signs of recent or ongoing major mergers, though subtle distortions or minor disturbances cannot be ruled out at this resolution. Overall, the galaxy seems to be a fairly massive system with modest star formation activity.
