The galaxy presents as a relatively smooth, round object. The central region is noticeably brighter and exhibits a yellowish-white hue, suggesting a population of older, less massive stars. The outer regions fade gradually into a diffuse halo with a more subtle color gradient and some indications of lower star density. There is no clear evidence of spiral arm structure or a prominent disk. The overall morphology suggests that the galaxy is an elliptical or possibly a lenticular galaxy viewed face-on, though the faintness of the outer region makes detailed classification challenging. Star formation is likely to be low within this object. No signs of major mergers are observed.
