The galaxy exhibits a complex morphology, possibly undergoing a merger or interaction. The primary body appears relatively smooth and concentrated, with a slightly elliptical shape. There is evidence of tidal features or disturbances emanating from the central region, suggesting gravitational interaction with another galaxy or a recent merger event. Two distinct regions of redder hue are visible in the vicinity of the central region, indicating potential areas of intense star formation or dust obscuration. The overall color profile of the galaxy suggests a population of older stars in the central bulge, with younger, bluer stars concentrated in the aforementioned regions. The galaxy's integrated light appears to be of intermediate luminosity, not exceptionally bright but also not a faint dwarf galaxy. The estimated size indicates a galaxy of substantial proportions, potentially comparable to the Milky Way in scale. Overall, this system appears to be a dynamic, evolving galaxy experiencing significant gravitational interactions and showcasing diverse stellar populations.
