The galaxy presents as a relatively compact object with a noticeable disk structure. While not a perfect spiral, some arm-like features are suggested by subtle variations in color and intensity. A general symmetry is observed about its core, suggesting a relatively undisturbed evolutionary history, though some minor irregularities may indicate past interactions. The galaxy’s central region appears brighter and more concentrated, indicating a significant stellar population and potentially an active galactic nucleus, although this cannot be confirmed from the image alone. Color gradients are apparent, with bluer hues in the outer disk regions, which could suggest ongoing star formation. Overall, the galaxy exhibits characteristics of a disk galaxy at an intermediate redshift, displaying both smooth and featured components in its morphology.
