The galaxy appears to be a relatively smooth, disk-shaped system, viewed at an angle. Its core exhibits a bright, concentrated luminosity, likely indicative of an older stellar population. Surrounding the core is a more diffuse disk. The disk shows a mottled appearance, with a greenish tint, suggestive of ongoing, but relatively subdued, star formation. There is no obvious spiral structure or bar, with the overall morphology leaning towards an elliptical galaxy but with the presence of a disk. There is no indication of a major merger event or significant tidal distortions. The galaxy exhibits a moderate redshift, suggesting it is at a considerable distance. The size of the galaxy appears typical for galaxies at its redshift, indicating it is likely a galaxy of substantial mass. Overall, the galaxy appears to be an intermediate-mass disk galaxy undergoing relatively quiescent star formation with an aging stellar population.
