The galaxy appears to be undergoing a merger event, possibly involving two or three distinct components. The primary body displays a diffuse, irregular morphology with a non-smooth, disturbed appearance, indicating potential gravitational interactions. The central region of the galaxy appears less defined, without a clearly visible bulge or nucleus. A plume-like extension emanates from one side, characterized by a yellowish hue suggestive of older stellar populations or dust obscuration. The main body of the galaxy exhibits a bluer color, indicating more recent star formation or a younger stellar population. There may be some tidal features present, suggesting the later stages of the merger. Star formation rate appears to be ongoing but at a relatively low level. Overall, the galaxy's morphology is indicative of a system in flux, influenced by ongoing gravitational interactions and a disturbed internal structure.
