The galaxy appears to be in the late stages of a merger. The galaxy's overall form is disturbed, and the smooth light distribution is more prominent than a spiral-like disk. There is evidence of two distinct nuclei, both with a yellowish hue. This suggests the presence of older stellar populations, but there may be some ongoing star formation as the galaxy's overall color appears somewhat blue. The galaxy is relatively compact. Overall, this galaxy's appearance indicates a system evolving towards a more spheroidal morphology.
