The galaxy presents as a relatively compact, elongated structure, seen nearly edge-on. The central bulge appears prominent and concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. Extending outwards from the bulge is a fainter, more diffuse disk. This disk component shows only subtle hints of internal structure; there is a possibility of faint dust lanes along the major axis. The galaxy's overall morphology is generally smooth, although some minor asymmetries may be present. There is no obvious evidence of recent major merger activity or significant tidal disruption. The color gradient from the bulge to the outer disk suggests some degree of on-going star formation. The inferred luminosity is relatively high for a galaxy at this redshift.
