This galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The galaxy exhibits a yellowish hue, suggesting an older stellar population with lower rates of star formation. The roundness of the galaxy indicates a low degree of flattening, characteristic of E0-E2 ellipticals. There is no obvious evidence of spiral arms or a disk structure. Additionally, there is no indication of major mergers or significant tidal disturbances. The galaxy appears largely undisturbed and isolated in its environment.
