The observed galaxy appears to be an interacting system, potentially in the late stages of a merger. Two distinct nuclei are visible, differing in color. The nucleus to the lower left is bluer in appearance, possibly indicating a region of active star formation. The nucleus to the upper right presents a yellower hue, suggesting an older stellar population. Both appear centrally concentrated and moderately smooth. There appears to be an absence of well-defined spiral arms or a prominent disk structure. Some degree of tidal disturbance is suspected, with what might be faint tidal tails or bridges hinted at in the surrounding diffuse light.
