The galaxy presents as a relatively smooth, centrally concentrated object with a roughly round morphology. There is a distinct central bulge which is brighter than the surrounding galactic disk or halo. There is little evidence of spiral arm structure or significant dust lanes. The color appears to be dominated by bluer wavelengths, suggesting a presence of younger, hotter stars, though the overall light distribution is rather uniform across the galaxy's extent. There is a subtle decrease in brightness as one moves outward from the galactic center, but the boundary of the galaxy appears diffuse, fading gradually into the background sky. No obvious signs of ongoing mergers or major disturbances are observed, although a minor asymmetry cannot be entirely ruled out. The smooth features suggest the galaxy is either an elliptical galaxy or a face-on disk galaxy with a substantial bulge component. 
