The galaxy presents as a relatively smooth object with a concentrated central bulge. The overall shape appears elliptical, exhibiting a moderate degree of roundness rather than a highly elongated form. There's a noticeable color gradient, with a yellowish-white core region that likely corresponds to an older stellar population. Surrounding the core, a bluer hue suggests the presence of younger, hotter stars, although these regions lack distinct spiral arm structures. The faintness and somewhat amorphous nature of the outer regions indicate a lack of significant ongoing star formation in the galaxy's periphery. While there are no obvious signs of major mergers or tidal disturbances, a subtle asymmetry in the outer halo cannot be ruled out.
