The galaxy appears as a centrally concentrated object with a diffuse halo. The core exhibits a bright, nearly spherical morphology with a noticeable blue hue, indicative of recent or ongoing star formation. The light distribution within the core suggests a possibly complex internal structure, with subtle variations in luminosity across its surface. A less luminous region to one side of the main body displays a distinctly bluer color, possibly signifying a region of intense star formation. Indications of a faint tidal feature, potentially a stellar stream or disrupted arm, are visible at the very edge of the galaxy, suggesting a possible past or current interaction with another galaxy, or perhaps a minor disturbance within the galaxy itself. The overall structure is suggestive of a galaxy undergoing or recently having undergone a merger event.
