The galaxy presents as a relatively smooth and elliptical structure, with a central bulge that appears bright and concentrated. The overall color is subtly reddish, suggesting a population of older stars. The galaxy appears to be viewed nearly edge-on, with a dust lane or obscuration possibly present along the major axis. There is little evidence of spiral arms or active star formation in this imaging, leading to the classification as a more mature galaxy. The galaxy does not appear to be undergoing any major merging events with other galaxies. The elliptical nature of this galaxy suggests a relatively high Sersic index. 
