The galaxy presents a somewhat amorphous morphology, dominated by a smooth, centrally concentrated light distribution. The color profile exhibits a yellowish hue, potentially indicative of an older stellar population or significant dust obscuration. There appear to be multiple nuclei present, suggesting either an ongoing merger event or a galaxy with a complex central structure such as a supermassive black hole or a double nucleus. Tidal features, if present, are faint or obscured, although the general light distribution hints at some gravitational disturbance. The galaxy appears to be relatively massive with modest star formation.
