The galaxy appears as an elongated, somewhat cigar-shaped structure. A central, bright bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy appear fainter and bluer in color, possibly indicating the presence of younger, hotter stars and ongoing star formation within a relatively flattened disk. No distinct spiral arm structure is readily discernible; instead, the light is more diffuse. The galaxy does not show any obvious signs of a major ongoing merger, but there is a minor level of asymmetry, potentially hinting at a past interaction or minor disturbance. Overall, it seems like a relatively massive galaxy at moderate redshift.
