This galaxy appears to be a disk galaxy, potentially a spiral galaxy seen at a slight angle. The central bulge exhibits a pronounced yellowish-red hue, suggesting an older stellar population. Fainter, bluer emission extends outwards from the bulge, indicating regions of ongoing star formation within the disk. The overall structure shows signs of potential minor disturbances, possibly from past interactions.  There is a significant amount of smoothness to the galaxy, suggesting that it may be undergoing a transition or a quenching of its star formation. The galaxy is relatively massive, and exhibits moderate star formation activity.
