The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall shape is largely elliptical and somewhat rounded, with a bright central bulge that gradually fades into the outer regions. There is no clear evidence of spiral arms or a distinct disk structure. Color gradients suggest the central region is composed of older stellar populations, as indicated by the yellower hue, while the outer regions are slightly bluer, potentially indicating the presence of some younger, star-forming regions. No significant tidal features or evidence of recent major mergers are visible. However, there are hints of minor disturbances in its morphology. Overall, it is likely an early-type galaxy undergoing some low-level star formation.
