The galaxy presents a morphology suggestive of an ongoing or recent merger event. Two distinct, bright nuclei are visible within a common, diffuse halo of stellar material. The nuclei appear roughly similar in luminosity, with slightly differing hues, suggesting potentially different stellar populations within each core. The overall shape of the galaxy is irregular, deviating significantly from a standard elliptical or spiral form, likely due to the gravitational interaction between the merging components. The presence of extended, faint tidal features or plumes are suspected within the halo, although not readily apparent, implying previous disturbances and redistribution of matter. The system exhibits a relatively smooth overall texture, with an inclination towards a round shape. Colors appear slightly redder than a typical spiral, possibly indicating an older stellar population.
