The galaxy presents as a disturbed system, likely undergoing a merger. Two distinct, bright nuclei are observed, suggestive of two interacting galaxies. The overall morphology is irregular, with faint tidal features potentially indicating gravitational interaction. The color of the galaxy is generally reddish, hinting at an older stellar population and moderate dust content, with only modest recent star formation. The observed roundness is intermediate, indicating a transition between spiral and elliptical morphology.
