The galaxy presents a complex morphology. The central region appears relatively smooth and unresolved, but the overall structure suggests the presence of disturbances. A faint, diffuse disk-like structure appears to extend outwards from the center. The disk exhibits variations in color and luminosity, with some regions appearing brighter and bluer than others. This could indicate ongoing star formation. I suspect a merger event with the galaxy based on subtle features like a potential tidal tail or plume extending away from the main body. The color composite suggests the presence of both younger, bluer stellar populations and older, redder populations within the galaxy.
