The galaxy presents as a somewhat elongated structure, indicative of a possible spiral or elliptical galaxy viewed at an oblique angle. The color distribution is not uniform; the central region appears more reddish, potentially indicating an older stellar population or significant dust obscuration. Fainter greenish hues extend outwards, especially at the edges, which could represent regions of more recent star formation or a younger stellar population. There are some very faint hints of spiral structure, but it cannot be confirmed based on this image. The galaxy exhibits a relatively smooth profile, suggesting a lack of major ongoing mergers or significant tidal disturbances. Overall, the galaxy seems to be a massive system with moderate star formation, and its form is reminiscent of a disk galaxy.
