The galaxy presents an overall distorted morphology suggestive of an ongoing or recent merger event. A primary, relatively smooth component dominates the structure. This component exhibits a yellowish hue, indicating an older stellar population. There is evidence of a second, smaller component appearing as a distinct but closely associated concentration of light with a slight orange tint. Faint tidal features or extended debris appear emanating from the main body of the galaxy, indicating gravitational interactions. The galaxy is not perfectly circular, but rather somewhat elongated. While the dominant portion appears relatively smooth, there are hints of internal structure within the distortion.
