The galaxy presents a disturbed morphology, suggestive of an ongoing or recent merger event. The overall form is irregular, exhibiting a somewhat elongated structure. Two distinct, relatively bright cores are visible, potentially representing the nuclei of the merging galaxies. There is a general smooth appearance with an absence of well-defined spiral arms or a prominent disk structure. The light distribution indicates a system dominated by older stellar populations, with lower levels of active star formation. A tidal tail or bridge-like feature appears to connect the two cores, further indicating gravitational interaction. The galaxy appears to be intermediate in size. Its shape is more in between than round, with a very slight lean towards a cigar shape. The merger is currently major, but the original galaxies show no major disturbance to their general shapes.
