The galaxy appears to be in the late stages of a merger event. Two distinct nuclei are visible, indicating the original cores of the merging galaxies. These nuclei exhibit a relatively smooth, rounded morphology. The overall color suggests an older stellar population, leaning towards redder wavelengths. Tidal tails or extended structures are not clearly visible, which may mean they are too faint to see or that the merger is advanced, and these features have dissipated. The merging galaxies could be experiencing a relatively low rate of star formation. The galaxy is of considerable mass.
