The galaxy appears to be a spiral type, viewed at an angle that is neither face-on nor edge-on. There's evidence of spiral arm structure, though the arms are not very well-defined. The color suggests ongoing star formation activity, particularly in the central regions and within the spiral arms, which exhibit a distinctly bluer hue. There is likely a bar feature present. The bulge component looks to be moderately small compared to the disk. Some level of tidal disruption may be observed.

