The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a slight elongation, but the overall morphology appears to be dominated by its spheroidal component, with a high degree of central concentration. The light distribution appears smooth and homogenous, suggesting an older stellar population. The galaxy has a subtle color gradient, appearing slightly bluer in the outer regions and redder toward the center. There is no obvious evidence of spiral arms, a disk component, or active star formation regions, which suggests that this galaxy is a relatively quiescent system. There appear to be no major tidal disturbances or merging features. The overall structure is undisturbed and shows no signs of significant interactions.
