The object appears to be a spiral galaxy at a distance, exhibiting a redshift of 0.2176. The galaxy presents a moderately inclined disk, with clearly visible spiral arms. The arm structure appears somewhat flocculent and disturbed, suggesting possible interactions. One arm is brighter than the other, which could be due to an ongoing disturbance or star formation. The galaxy possesses a moderately sized bulge, and has no visible bar structure. The galaxy has an apparent blueish colour, indicating a possibility of ongoing star formation. The overall morphology hints at potential merging activity or interactions with other nearby galaxies, although a clear merging event is not apparent in this image. The dust lanes are not prominently visible, which suggests the galaxy may be viewed at a higher inclination angle relative to its disk plane. The overall light distribution indicates a dominant disk and possibly some recent interaction which is indicated by the disturbed spiral arm structure.
