The galaxy presents as a centrally concentrated system with a relatively smooth overall morphology. There is a distinct bright, yellowish core suggesting an older stellar population dominating the central bulge. Moving outward from the core, a gradual transition to a more diffuse, bluish halo is observed. The overall shape appears generally elliptical with a slight elongation, leaning towards an in-between roundness. No prominent spiral arms or significant dust lanes are discernible in this image, which further supports classification as a relatively smooth system. The observed color gradient, with a redder center and bluer outer regions, likely indicates radial variations in the stellar populations and ongoing star formation activity concentrated in the outer disk. No signs of major tidal disturbances or mergers are visible, suggesting relative quiescence in its recent history.
