The target galaxy presents a predominantly smooth morphology, with a significant central bulge. The light distribution indicates a relatively low level of ongoing star formation. There is evidence of disk structure, though it is not sharply defined. There is no signs of tidal tails or strong interactions, although there are some hints of minor disturbances. The color gradients suggest a stellar population that is slightly redder in the central regions, becoming bluer further out. Overall, the galaxy appears to be a relatively undisturbed system.