The galaxy presents as a moderately luminous object at a redshift of approximately 0.16, indicating a significant distance. Morphologically, the galaxy exhibits signs of a possible ongoing or recent merger event. A significant portion of the galaxy light seems concentrated in two primary, slightly elongated regions or components. These two features appear connected by a faint bridge of light, hinting at a possible tidal interaction. There are some minor disturbances to the morphology suggesting some kind of interactions. The galaxy exhibits a predominantly smooth appearance with minimal evidence of spiral arm structure. The colors are relatively uniform, indicating an aging stellar population with suppressed current star formation. There appears to be no dust lane structure visible. Overall, the object has a diffuse and disturbed appearance consistent with a galaxy involved in a gravitational interaction or recent merger.
