The galaxy presents as a smooth, elliptical form with a concentrated central bulge. The light distribution is relatively even, exhibiting a gradual decrease in intensity from the core outward. The galaxy's color appears to be dominated by yellow and red wavelengths, suggesting an older stellar population with lower star formation rates. There's no evident spiral structure or significant dust lanes. Faint irregularities may be present along its outer edges, hinting at potential minor tidal interactions or past merger events. The overall morphology indicates a relatively evolved system nearing the end of its star-forming lifecycle.
