The galaxy presents as a centrally concentrated object with a generally smooth appearance. The central region exhibits a bright, yellowish hue, likely indicating an older stellar population and reduced ongoing star formation. Surrounding this core is a more diffuse, bluish halo. This bluer color suggests the presence of younger stars or regions of active star formation, although these regions are not clearly resolved into distinct structures. The overall morphology appears to be a system without obvious spiral arms or a well-defined disk, with some indication of tidal disturbances or a merger.
