The galaxy presents as a distorted disk structure, suggesting possible ongoing or recent interaction/merger events. There is a central bulge with a relatively bright core, surrounded by a flattened disk component. The disk appears disturbed, exhibiting asymmetries and possibly tidal features or plumes extending from the main body of the galaxy. The overall color of the galaxy is bluish-white, indicative of a population of younger, hotter stars, especially in the disk. However, there's also evidence of older stellar populations contributing to the light in the bulge. The shape is not perfectly round, showing more of an elongated form with irregularities. There is some suggestion of active star formation, with brighter, bluer regions scattered across the disk, though it seems concentrated in certain areas rather than uniformly distributed. There may be evidence of dust lanes obscuring some of the light from the bulge, but it is not definitive. Overall the galaxy shows signs of a system undergoing dynamic changes with potentially ongoing interactions or recent merger events.
