The galaxy presents as a somewhat elongated, elliptical morphology. The central region exhibits a higher concentration of light, suggestive of a bulge. The color profile is dominated by yellow-red hues in the core, potentially indicating an older stellar population. Fainter, blue-ish outskirts can be seen, possibly representing regions of more recent, albeit relatively low, star formation activity or a population of younger stars. There is no clear evidence of spiral arm structures. The galaxy appears relatively undisturbed, without any indications of major mergers or significant tidal disruptions. It possesses a smooth overall appearance. The galaxy may be located at a significant distance, given its faint appearance, consistent with its measured redshift.
