The galaxy appears to be undergoing a significant interaction or merger. Two distinct, bright cores are visible, suggesting the presence of two progenitor galaxies. These cores are embedded in a larger, diffuse halo of light. The overall morphology is highly disturbed, with irregular shapes and tidal features indicating gravitational disruption. There are no clear spiral arms or a well-defined disk. The color gradient shifts from reddish hues in the central regions towards a bluer tinge in the outer areas of the halo, possibly indicating differing stellar populations or dust extinction levels across the system. The overall impression is of a system far from gravitational equilibrium. The estimated size is a radius of roughly 9 kpc.
