The object presents as a galaxy undergoing an apparent merger or interaction. There are multiple distinct components, suggesting a complex structure. One component appears as a somewhat elongated disk with hints of spiral arms. This region exhibits a yellowish-green hue, possibly indicating a population of older stars. The disk appears disrupted, showing tidal tails. Another distinct component shows bluer colors, which is indicative of active star formation. This area is less defined in its structure, suggesting that it is heavily disturbed by the interaction. The third component also seems to contain a ring-like structure with reddish concentrations, possibly indicative of dust lanes. The overall morphology indicates significant gravitational interaction between two or more galactic bodies, leading to ongoing structural deformation and star formation. The galaxy exhibits a moderately bright appearance, suggesting relatively close proximity or high intrinsic luminosity.
