The galaxy presents as a system undergoing an apparent merger or significant interaction. Its overall shape appears disturbed, deviating from a regular elliptical or spiral morphology. There is a prominent, bright central region with a yellowish hue, suggesting an older stellar population, perhaps a bulge. Extending from the main body is a diffuse, elongated structure with a slightly bluer tint, indicating the presence of younger stars and potentially ongoing star formation, possibly tidally induced. There's indication of a faint, connecting bridge or tail-like feature extending to a secondary object. The morphology suggests a major merging event is in progress, supported by observed disturbances.
