The galaxy appears to be a spiral galaxy at a redshift of approximately 0.2, indicating a significant distance. Its morphology suggests some level of disturbance or interaction, as evidenced by the asymmetry in its spiral arms and the presence of a tidal tail-like feature extending from one side. The galaxy exhibits a relatively bright, concentrated central bulge, which is yellow, indicating an older stellar population. The spiral arms show bluer hues, suggesting ongoing star formation within these regions. There is a small, blue, diffuse region towards the end of its disturbed tail. Overall, the galaxy seems to be undergoing some form of evolutionary process, possibly due to a minor merger or gravitational interaction with another galaxy.
