This galaxy presents as a moderately extended object, appearing slightly elongated in shape. The color gradient suggests a complex composition. There is a central, brighter region that is slightly more red-toned which could indicate an older stellar population or the presence of dust. Fainter, blue-ish regions are observed on both sides of the central area, possibly indicating areas of active star formation. Overall the galaxy appears to be relatively smooth in texture, with little indication of defined spiral arms or a prominent central bulge. The faintness and irregular morphology may suggest a more distant galaxy, possibly undergoing some form of interaction or disturbance, given that there is some evidence of merging or minor disturbance. 
