The galaxy presents as a moderately inclined spiral, potentially a late-type spiral based on the loosely defined arm structure and clumpy nature of the disk. The central bulge is not prominent, suggesting a smaller mass concentration at the core. The color profile appears relatively uniform across the galaxy, trending towards a bluer hue which might be caused by the redshift. There is some indication of ongoing star formation within the disk, evidenced by localized brighter regions. No obvious signs of major mergers are observed, though minor disturbances or interactions cannot be ruled out given the irregular morphology and presence of potential tidal features. The overall morphology suggests a stable, relatively undisturbed spiral galaxy undergoing moderate star formation.
