The galaxy presents as a spiral type, exhibiting a clear disk structure. The spiral arms are tightly wound and display a prominent presence with a defined, but not overly prominent structure. The arms appear to be populated with regions of active star formation, indicated by the blotchy blue-ish coloring observed in the disk. A central bulge is visible. There appears to be a slight warp or asymmetry to the disk. The nucleus of the galaxy is bright and distinct, likely indicating the presence of a supermassive black hole that is actively accreting material. There is no apparent sign of any tidal disruption indicating a past major merger.
