The galaxy presents a disturbed morphology, suggestive of a possible merger event or significant tidal interaction. The primary body of the galaxy appears relatively smooth and elliptical, with a concentration of light in the central region, likely indicative of an older stellar population. There is evidence of a distinct, bluer, less concentrated region offset from the main body, possibly indicating an area of active star formation. The overall shape is somewhat elongated, with a hint of asymmetry. The color gradient suggests a transition from younger, bluer stars in the disrupted region to older, redder stars in the core. There is a small fraction of merging present, with the larger fraction being no merger at all.
