The galaxy exhibits a disturbed morphology, indicative of potential interactions. A central, bright core is visible, surrounded by a disk-like structure. The disk displays irregularities; there is a noticeable asymmetry and a possible tidal tail, which may be evidence of a minor merger event. There is a suggestion of a spiral arm-like structure, though it is not well-defined. Dust lanes are present throughout the galaxy, obscuring some of the light. The overall color of the galaxy appears to be consistent across its structure, with an enhanced intensity within the core, signaling a relatively consistent stellar population, but there is a very slight blue shift in the northern region. The galaxy's brightness decreases with distance from the center.
