The galaxy presents a largely smooth, elliptical morphology. A discernible central bulge is observed with a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy appear less concentrated with a slightly bluer color gradient, potentially indicating the presence of younger stars or ongoing star formation, although to a low degree. The galaxy exhibits a relatively regular shape, with no obvious signs of tidal disturbances or major ongoing mergers. Some minor disturbances can not be ruled out. The galaxy is not perfectly spherical and appears more intermediate in shape, and it is likely not disk shaped. Overall, the galaxy appears to be a fairly evolved system with a dominant spheroidal component.
