The galaxy presents a largely smooth morphology. The overall shape appears elliptical, exhibiting high degree of circularity. There is a distinct central bulge with a higher concentration of luminosity. The color gradient suggests an older stellar population, particularly within the bulge, with a shift towards redder wavelengths. Evidence of a prominent disk structure or spiral arms is not readily apparent. No clear signs of ongoing major mergers or significant tidal disturbances are visible. The outer regions of the galaxy gradually fade, suggesting a fairly smooth density profile.
