The galaxy presents a relatively smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decrease in intensity towards the outer regions. The galaxy exhibits a color gradient, with a yellowish-white core transitioning to a bluer halo. There is no discernable spiral arm structure or significant dust lane obscuration apparent. There is a slight deviation from perfect circularity, suggesting that the galaxy is an elliptical galaxy with a ratio close to 1. It also appears to have a slightly disturbed form suggesting that it had some minor disturbances within its past. Overall, this galaxy seems to be relatively massive, given the high luminosity, and exhibiting a modest amount of star formation.
