The galaxy presents a complex morphological structure, exhibiting characteristics of both smooth and featured components. The galaxy's central region appears relatively smooth, suggesting a possible elliptical or lenticular morphology. However, there are clear signs of disturbance or features extending from the central region. These features, while not pronounced spiral arms, indicate some degree of disk-like structure or tidal interaction. 

The color gradient across the galaxy shows a bluer hue towards the outer regions. This suggests ongoing star formation within the galaxy. The galaxy's intermediate roundness implies neither a perfectly spherical nor a highly elongated shape, but rather an in-between morphology. Evidence suggests the galaxy could be undergoing a merging process, with signs of tidal disturbances possibly due to a minor merger. The galaxy's estimated size is consistent with a moderate-sized galaxy at its redshift.
