The galaxy presents as a relatively smooth, elongated structure, suggestive of an edge-on or highly inclined disk. The central region appears brighter and more concentrated, exhibiting a yellowish-orange hue indicative of an older stellar population. Fainter, bluer regions extend outward from the central bulge, hinting at ongoing or recent star formation within the disk. The overall morphology is largely undisturbed, without clear evidence of major mergers or tidal interactions, although some minor asymmetry is visible within the disk. The galaxy is estimated to have a moderate stellar mass and a moderate star formation rate, suggesting it is a fairly typical star-forming galaxy at its redshift.