The galaxy presents a generally smooth morphology, appearing largely spheroidal with a diffuse halo. There is a distinct central bulge, characterized by a concentrated luminosity gradient. Color gradients suggest a redder core, possibly indicating an older stellar population, with a bluer, less concentrated, outer halo. There is a subtle asymmetry in the distribution of light in the outer regions but no clear signs of spiral arms or other disk-like structures, nor strong tidal disturbance that might indicate an ongoing merger. Overall, it shows a typical elliptical galaxy morphology.
