The galaxy exhibits a disturbed morphology, potentially indicating a recent or ongoing merger event. There appear to be two distinct nuclei, one with a reddish-orange hue and the other displaying a bluer coloration. A significant portion of the galaxy's light is concentrated in these two regions. The overall shape is irregular, deviating from a simple elliptical or spiral structure. The reddish nucleus may indicate an older stellar population or significant dust obscuration, while the blue nucleus could be indicative of ongoing star formation. Tidal features, though not prominently displayed, may be subtle indicators of the gravitational interaction between the merging components. The galaxy appears relatively compact.
