The observed galaxy appears as a merging system, with two distinct, luminous components exhibiting evidence of gravitational interaction. The primary body displays a yellowish-white hue, with a smooth, rounded morphology indicating a relatively evolved stellar population. The secondary body, located in close proximity, exhibits a similar yellowish color. There is clear indication of tidal disturbances between the galaxies, the system has a relatively compact structure, and the overall light distribution suggests that the system is dominated by an older stellar population, with little active star formation. The galaxy shows relatively little structure outside of the two bodies, and is generally smooth, with a faint color and low star formation rate.
