The galaxy presents as a system undergoing a significant merger or interaction. There appear to be at least two distinct nuclei or regions of high stellar density, one more luminous and compact than the other. A diffuse, irregular halo or envelope surrounds these central components, exhibiting faint tidal features and streamers. The color gradient suggests a complex stellar population, with bluer hues possibly indicating areas of recent or ongoing star formation within the disturbed structure. The overall morphology deviates significantly from a standard elliptical or spiral form, instead showcasing an amorphous and perturbed shape indicative of gravitational disruption.
