The observed galaxy presents as an edge-on or highly inclined disk galaxy. There is a distinct central bulge, appearing a yellow-white hue, which indicates a concentrated population of older stars. The galactic disk itself exhibits a blue-white colour. It's general morphology suggests ongoing star formation. The structure seems relatively undisturbed, with no obvious signs of major mergers or tidal disruptions. However, there is some subtle indication of minor asymmetry, suggesting it might be experiencing a minor interaction. The estimated physical radius of the galaxy is approximately 4 kpc. Overall the galaxy appears to be relatively massive and actively forming stars.
