The galaxy presents as a system undergoing a merger. Two distinct luminous regions are observed, one exhibiting a more reddish hue, and the other a more yellow color. The larger, redder component appears relatively smooth and featureless, while the smaller, more yellow component shows some irregularities. A faint, diffuse, blueish structure is visible to the side. There is potential morphological disturbance indicative of gravitational interaction with the other component. Based on the morphology, the system may be approaching, or is in the process of complete merging. Overall the galaxy has an estimated mass around 10^11 solar masses.
