The galaxy presents an overall elliptical morphology. It appears largely smooth in structure, lacking prominent spiral arms or significant dust lanes. There is a central concentration of light, suggesting a prominent bulge. The color gradient shifts from a reddish core to a slightly bluer halo, which indicates a more evolved stellar population concentrated in the center, and younger star formation in the outer regions. There is no strong evidence of an active galactic nucleus, and it seems this galaxy is not currently undergoing major disturbances.