The galaxy appears to be a relatively smooth, elliptical galaxy, with a concentrated central bulge. It displays a nearly spheroidal shape, with a high degree of roundness. There is little to no visible disk structure or spiral arm features. The light distribution suggests a centrally concentrated stellar population. There are no clear signs of ongoing major mergers or significant tidal disturbances. The galaxy appears to be relatively isolated and unperturbed in its morphology. Color gradients suggest that the central region may be slightly redder than the outer regions, potentially indicating a more evolved stellar population in the core. No dust lanes or significant star-forming regions are apparent.