The galaxy appears as a lenticular or early-type spiral galaxy, observed at a redshift suggesting a considerable distance. It exhibits a relatively smooth morphology, with a noticeable disk-like structure. The central bulge is somewhat prominent, with a luminosity gradient that appears to decline smoothly outwards, indicating a well-established stellar population. There may be some subtle, faint features within the disk, though they are not sharply defined, suggesting a more evolved and less active state of star formation, though there may still be some activity. There is little evidence of significant recent or ongoing major mergers or tidal disturbances; however, some minor disturbance cannot be ruled out. The galaxy's color suggests a mix of stellar populations, with some regions potentially dominated by older, redder stars and others with relatively young stars that contribute to a blueish hue.
