The galaxy exhibits a complex morphology, possibly indicative of an ongoing or recent merger event. The primary structure appears to be composed of at least two distinct components, one is more diffuse with a more pronounced yellow hue, while the other is more defined. There is also a third object with a smaller, dimmer profile. The overall color gradient suggests varying stellar populations, with the yellowish hues pointing towards older stellar populations or significant dust obscuration. The lack of well-defined spiral arms suggests an elliptical, lenticular, or disturbed disk galaxy type. The relative size and shape indicates that the galaxy is likely an intermediate mass system. Further spectroscopic analysis is required to confirm the star formation rate and the age of the stellar populations within the galaxy. The irregular morphology warrants further investigation into potential tidal features or interactions with nearby galaxies.
