The object presents as an edge-on disk galaxy at a redshift indicating a significant distance. It exhibits a prominent central bulge, characterized by a yellowish hue, suggesting a population of older stars. The disk component appears elongated and somewhat thinner, displaying a redder color, possibly indicative of dust lanes obscuring some regions. The overall structure suggests a relatively smooth morphology, with little evidence of major ongoing mergers or significant tidal disturbances. While no obvious spiral arm structures are visible, the disk component shows some features or irregularities, suggesting it may be a late type spiral galaxy that is highly tilted to our line of sight.
