This galaxy appears to be a spiral galaxy, observed at an inclination that is neither face-on nor edge-on. It exhibits a disk-like structure with subtle spiral arm features. The spiral arms are not particularly well-defined, giving the galaxy a somewhat flocculent appearance.

A central bulge is present but not dominant. There's no strong bar structure visible. The galaxy appears to be undergoing some form of interaction or disturbance, as indicated by the overall irregular shape and the presence of potential tidal features or distorted arm segments.

The color gradient suggests ongoing star formation, with bluer regions likely indicating areas of more intense star formation activity. The redder regions may correspond to older stellar populations or areas obscured by dust. The overall appearance indicates a galaxy with moderate mass and a moderate rate of star formation. There is no apparent presence of an AGN.
