The galaxy presents as a disk galaxy, likely a spiral, though the image quality and viewing angle obscure prominent spiral arm features. A central bulge is visible, appearing yellowish-white in color, suggesting an older stellar population with lower star formation. The disk component has a bluer hue compared to the bulge, potentially indicating ongoing star formation in the disk. Some subtle structures within the disk are visible; slightly brighter regions may represent areas of active star formation. The overall smoothness of the galaxy's light distribution suggests that this galaxy could be a relatively undisturbed system. There seems to be evidence of some dust, but that is not for certain. The observed redshift indicates that this galaxy is at a considerable cosmological distance, but not extraordinarily high.
