The observed galaxy presents as a disk galaxy, exhibiting a prominent and relatively well-defined galactic plane. The overall color profile suggests a mixture of stellar populations. There's a noticeable concentration of bluer light particularly along one side of the disk, potentially indicating ongoing star formation. In comparison, the opposite edge of the disk appears less defined and a lighter color, hinting at a possibly older stellar population or dust obscuration.

We see some areas of disturbance in the galactic disk, possibly indicating minor interactions. There does not appear to be a dominant central bulge, though some increased central light concentration exists. A slight irregularity along one edge of the disk also suggests tidal interactions or past merger events. Overall, the galaxy exhibits a disk structure with ongoing processes of star formation and potential morphological disturbances.
