The galaxy presents as an elongated, disk-like structure with a clearly defined central bulge. The color profile suggests an older stellar population concentrated in the bulge, exhibiting a yellowish-orange hue. Fainter bluish light extends from the central bulge into the disk, possibly indicating regions of ongoing star formation. The disk appears relatively smooth with some irregularities in the light distribution, which may be indications of spiral arm structures or dust lanes, though they are not sharply defined in this image. There is no obvious sign of a recent major merger event or tidal disturbances, although subtle asymmetries are present within the disk structure. Overall, the galaxy appears to be a relatively massive spiral galaxy at moderate redshift.
