The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. Its overall color appears bluish-white, suggestive of a population of hotter, younger stars. There is no clear evidence of distinct spiral arms or a prominent disk structure. The light profile seems to fade gradually from the central core outwards, lacking sharp edges or features indicative of significant recent merger activity, although a subtle asymmetry may be present. The morphology is most consistent with an elliptical or lenticular galaxy, likely at an intermediate redshift.
