The galaxy presents a predominantly elliptical morphology with a smooth, centrally concentrated luminosity profile. It exhibits a yellowish-orange core, suggestive of an older stellar population likely dominating the central region. The outer regions display a bluer hue, potentially indicating the presence of younger stars and ongoing or recent star formation. There's a subtle suggestion of a disk-like component, though not sharply defined. There also appears to be some form of disturbance, or a merging event occurring within the galaxy.
