The galaxy presents a somewhat disturbed morphology, potentially indicating an ongoing or recent interaction. The central region exhibits a moderate concentration of light, with a slightly elongated appearance. There are hints of faint tidal features or asymmetries in the outer regions.

Color gradients suggest a mixture of stellar populations. The bluer colors on the outskirts could indicate younger stars and active star formation, while the more central, reddish hues likely correspond to an older stellar population. 

The galaxy appears to be relatively compact. Overall, this galaxy seems to be in an intermediate stage of evolution, possibly transitioning from a disk-dominated to a more spheroidal system.
