The galaxy presents an elongated morphology, seemingly transitioning between elliptical and cigar-shaped. Its central region exhibits a concentrated brightness, indicating a possible active galactic nucleus or a region of intense star formation. A smooth, diffuse halo surrounds this central core, yet some visible internal structure suggests ongoing interactions or mergers. Distinct tidal tails and disturbances are present. These tails indicate recent or ongoing gravitational interactions, potentially with smaller satellite galaxies or other nearby galaxies. The presence of these tails also suggests that the system may be dynamically young, still settling after a merger event. The galaxy's overall color appears bluish, suggesting the presence of younger, hotter stars. Patches of more green tinted regions are scattered across the galaxy, possibly caused by the presence of ionized gas or areas of active star formation. These regions might be associated with the disturbances and tidal features, indicating triggered star formation from the interaction. The overall light distribution suggests a system that is far from relaxed, actively evolving due to ongoing interactions.
