The galaxy presents a complex morphology suggestive of a system undergoing a merger. Two distinct luminous components are observed. One component exhibits a relatively smooth, round appearance, with a diffuse and uniform light distribution. Its color is predominantly redder, indicating an older stellar population. The second component appears more disturbed and irregular, with a bluer color suggesting the presence of younger, hotter stars and potentially ongoing star formation. There is a hint of tidal features that extend outward, indicative of gravitational interaction between the two components. The overall system lacks a clearly defined spiral or elliptical structure. A significant portion of the light appears concentrated towards the central regions of each component, though the system is not particularly luminous.
