The galaxy exhibits a complex morphology, potentially indicative of an ongoing or recent interaction. A significant portion of the galaxy's light is concentrated in a smooth, centrally located bulge or core. This core appears slightly elongated. A fainter arm or tidal tail extends outwards, showing signs of structural disturbance. The color distribution shows a concentration of yellow/red light in the central region, perhaps indicating an older stellar population, while the outer structures show areas of bluer light, which may be regions of more recent star formation. The overall appearance suggests a galaxy with a substantial old stellar population undergoing some form of interaction that is stimulating new star formation in certain regions.
