The galaxy presents as a system undergoing a significant merger event. The morphology is highly disturbed, with evidence of multiple interacting components. A dominant central mass appears to be coalescing, exhibiting a somewhat rounded, though irregular, central region. Faint tidal features are visible, extending outwards from the primary mass. These extensions suggest strong gravitational interactions and disrupted stellar populations. There is one major and one minor disturbance. The object exhibits a general yellowish-red hue, suggesting an older stellar population possibly obscured by dust, yet indicates that the merger may be inducing ongoing star formation activity, particularly given its apparent luminosity. The estimated size of the galaxy is about 10 kpc.