This galaxy presents as a spiral type, though with a notable degree of fuzziness, possibly indicative of a higher redshift or significant dust obscuration. The central bulge is clearly visible and appears moderately sized, exhibiting a yellowish hue, suggestive of an older stellar population. Two spiral arms originate from the core region, with a tightly wound morphology. The disk appears relatively large, with a high degree of axial symmetry. Patches of bluer light are observed within the spiral arms, potentially signifying regions of active star formation. There does not appear to be any major merging events, and the structure is well-formed and symmetrical.
