The galaxy appears as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The light distribution suggests an older stellar population, with a dominant redder hue across the galaxy, indicating lower levels of recent star formation. There is little evidence of spiral arms or a distinct disk component. The galaxy seems relatively undisturbed, showing no significant signs of ongoing mergers or tidal interactions with neighboring galaxies.
