The galaxy presents as a system undergoing a potential merger event. The overall morphology suggests a generally smooth structure, but with notable disturbances. There's a primary, more diffuse component, and a secondary, more compact and luminous region suggestive of a galactic nucleus or the core of an infalling galaxy. The colour gradient indicates ongoing star formation, particularly in the more compact region, which appears redder, likely due to dust obscuration or a population of older stars. There is some evidence of tidal features or distortions in the outer regions of the system, though they are not pronounced. A faint halo surrounds the main body of the galaxy. The system does not appear to be highly inclined, as the shape appears relatively circular.
