The galaxy presents as a somewhat elongated, cigar-shaped structure. It displays a largely smooth morphology with a concentrated central bulge or core that gradually diffuses outwards. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating, potentially indicating lower star formation activity. There is no clear evidence of prominent spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of major merging events or tidal distortions. The apparent lack of distinct features could also be due to the galaxy's high redshift.
