The galaxy exhibits a morphology indicative of an ongoing or recent merger event. Two distinct luminous components are visible, suggesting two separate galactic nuclei in close proximity. The overall structure is disturbed, lacking a clear spiral or elliptical form, and exhibits tidal features or distortions. The color of the galaxy is generally reddish/yellowish, suggestive of an older stellar population with relatively low ongoing star formation. The galaxy has a relatively high luminosity, likely due to the combined light from both merging galaxies.
