The galaxy appears to be a spiral galaxy exhibiting a disk-like morphology with a moderate bulge. The disk component shows evidence of spiral arm structure, although not sharply defined, with some regions of bluer light suggestive of ongoing star formation. A strong central bar structure is suspected. The overall color suggests a mix of stellar populations, with a redder bulge indicating older stars, and bluer spiral arms possibly denoting younger stars. There is no major disruption to the spiral structure, but there may be some minor tidal disturbances that are very faint. The galaxy has an estimated redshift value suggesting that it is relatively far away and being observed as it existed several billion years ago.
