The galaxy presents as a relatively smooth, elliptical morphology. There is a concentrated central bulge, and it exhibits a yellowish hue, indicative of an older stellar population with lower rates of ongoing star formation. The galaxy appears to be fairly isolated, showing no prominent signs of major interactions or mergers. The shape leans towards a spheroid, only slightly elongated. Any potential spiral arm structure is not visible, likely due to its type, high redshift, and the limitations of the image resolution.
