This galaxy presents as an apparent interacting system, possibly in the late stages of a merger. The overall form is elongated with a central concentration of light, appearing somewhat disturbed and irregular. Two prominent, relatively bright knots of light are visible within the system, one appearing more centrally located and the other slightly offset. These may represent the remnant cores of the progenitor galaxies. The system exhibits a yellow-reddish hue, suggesting an older stellar population, and potentially indicating lower rates of star formation. There is some evidence of tidal features or distortions, albeit subtle, potentially pointing to ongoing gravitational interactions. The galaxy's morphology suggests it is transitioning from a disk or spiral-like structure to a more elliptical or irregular form.
