This galaxy presents as a relatively luminous system with a slightly elliptical morphology. The central region exhibits a bright, concentrated core, suggestive of a significant stellar density, likely an aging stellar population.

The galaxy displays a prominent, extended disk surrounding the central core. The disk exhibits a bluer hue compared to the core, hinting at ongoing star formation. The overall structure appears relatively undisturbed, although subtle irregularities in the outer regions of the disk might indicate minor gravitational interactions.

Overall, this appears to be a substantial galaxy that has been classified by others as smooth, with some features of a disk-like structure, at a distance implied by its redshift.
