The observed galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on from our line of sight. A prominent central bulge is apparent, with a morphology that appears somewhat rounded, though a boxy structure is also observed, indicating a possible bar or structural instability within the bulge.

The galactic disk exhibits a relatively smooth texture, suggesting that the galaxy is not currently undergoing a major merging event or significant star formation. However, slight color variations are observed across the disk, potentially indicative of differential stellar populations or dust lanes obscuring regions within the disk. The galaxy does not show evidence of significant tidal features or other major disturbances, further suggesting a relatively quiescent state. The red shift suggests the galaxy is not a nearby galaxy. 
