The galaxy presents a predominantly smooth morphology, exhibiting a high degree of radial symmetry. It is largely elliptical, with a high degree of roundness, and minimal apparent disk structure. There is no noticeable bar or spiral arm structure. Color gradients suggest a relatively older stellar population, with an orangish hue. The galaxy's light distribution is concentrated toward the center, indicative of a centrally dominant bulge. There are no clear signs of ongoing major mergers or significant tidal disturbances, although a slight asymmetry in the outer regions cannot be completely ruled out. Overall, it appears to be an evolved, relatively quiescent system.
