The galaxy presents a predominantly smooth, elliptical morphology. The light distribution appears centrally concentrated with a generally round shape. There is a subtle hint of bluer hues concentrated towards one side, suggesting potential regions of ongoing, albeit moderate, star formation activity. The lack of obvious spiral arms or significant dust lanes points towards a more evolved stellar population. No major merger events or strong tidal disturbances are readily apparent in the immediate vicinity of the galaxy, which indicates that interactions with other galaxies have not significantly impacted its current structure. The overall appearance is consistent with a massive elliptical galaxy at an intermediate redshift.
