The observed galaxy appears to be a spiral galaxy, seen edge-on from our perspective. A prominent dust lane bisects the galaxy, obscuring the galactic center, but the galaxy is a disk galaxy. There is a central bulge, which appears to be a mix of redder light. This implies a region populated by older stars. The disk component is bluer in color, suggesting ongoing star formation and a younger stellar population. This disk material appears patchy and non-uniform. There is no evidence of a strong tidal disturbance or major merger events. The galaxy may be undergoing only minor interactions or may be isolated.
