The observed galaxy presents a complex morphology suggestive of an ongoing or recent merger event. It appears as a system of two distinct, bright components, likely representing the cores of the merging galaxies. Both components exhibit a somewhat elliptical shape, with a yellow-orange hue, potentially indicative of an older stellar population. There is faint, disturbed emission between the two components, possibly a tidal bridge. Based on the red color, the star formation rate of this galaxy appears to be low. The galaxy exhibits a moderately smooth appearance overall, with some evidence of disturbance.
