This galaxy exhibits an overall elliptical morphology with a prominent, concentrated central bulge. The bulge region appears yellowish-orange, suggesting a population of older, redder stars. The galaxy's outer regions show a gradual decline in luminosity, appearing smoother with a hint of blue; some evidence of disk-like structure might be present. There is no clear evidence of spiral arms or significant dust lanes within the galaxy. The galaxy appears relatively isolated, without any obvious signs of tidal interactions or ongoing mergers. The colors imply a galaxy whose stellar formation has largely ceased, but some low-level star formation may still be present in the outer regions.
